R      AND    S 5/4.5 E.
S      AND    SN (NGC 224).
W      AND    S 7.5/1-E.
X      AND    S 5/7-E.
Z      AND    KPBA ECKA XAPAKTEPETC BCKAM
              O 4M, PAEEHHM HTEPBAAM B 1-2 ECT-
              KA ET. B POMETKAX HAATC KEC-
              KE KOEAH ECKA CO CPEHM EPOOM
              632D  BOHOOPAHE MEHEH C KAM B
              HECKOKO HE  DM-0.1M-0.5M. CEKTP KOM-
              HPOBAHH, C PHAKAM AHTA OHEO
              KACCA M, KM MCCOHHM HM H-
              KOO BOEH (BL EQ)  APEEHHM -
              HM, XAPAKTEPHM  BCOKOBOEHHX
              TMAHHOCTE./THE LIGHT CURVE IS CHARACTERIZED
              BY OUTBURSTS UP TO 4M WITH INTERVALS OF 10-20
              YEARS. IN THE INTERVALS CYCLIC VARIATIONS ARE OB-
              SERVED WITH THE MEAN PERIOD OF 632D AND VARIATI-
              ONS WITH CYCLES OF SEVERAL DAYS AND DM-0.1M-
              0.5M. THE SPECTRUM IS SYMBIOTIC, WITH FEATURES
              OF A LATE M GIANT, NARROW LOW-EXCITATION EMISSION
              LINES (BL EQ) AND FORBIDDEN LINES CHARACTERISTIC
              OF HIGHLY EXCITED NEBULAE.
RR     AND    S 6/3.5 E.
RT     AND    MIN II 8.88; DI=DII=0.17P; DI=DII=0.00. P VAR. HE-
              HEH EH:/NONLINEAR TERM:-6.33*10**-11*E**2.
              B HTEPBAE/DURING J.D.2433477-43878 OB-
              ETBOPTEHE HEHE EMEHT:/LINEAR ELE-
              MENTS ARE SATISFACTORY: MIN=2441141.8888+
              +0.62892984D*E. BOMOHO, MEHEH EPOA HO-
              CT CHCOAH XAPAKTEP/PERIOD CHANGES
              ACCORDING TO A SINE LAW ARE POSSIBLE  8002!.
RU     AND    P VAR. MAX=2419857+243.0D*E (J.D.2412800-
              20000); MAX=2434551+233.24D*E*(J.D.2420000-
              34550). OCE/SINCE J.D.2435000-CM.TA./
              SEE TABLE. DM-4M-5M (O/BEFORE J.D.2429600),
              -1M (J.D.2429600-33600), O/UP TO 3M (J.D.-
              2436000), -1.5M (J.D.-2436700). B 1970-1972
              MEHAC COBCEM XAOTECK./IN 1970-1972
              SHOWED QUITE IRREGULAR VARIATIONS.
RX     AND    SB (P=0.21173D). OCE HOPMAHOO MAKCM-
              MA HAAC KBAEPOECKE CA-
               C P-38S-54S, OCE KOPOTKOO MAKCM-
              MA EPOHOCT HE HAAOC  8004!./
              CYCLIC VARIATIONS WITH P-38S-54S WERE OBSER-
              VED AFTER A NORMAL MAXIMUM; AFTER A SHORT MAXI-
              MUM NO PERIODICITY WAS FOUND  8004!.
SS     AND    HAATC TAKE EE BA OOEPOEC-
              KX KOEAH:/TWO LONG PERIOD VARIATIONS ARE
              ALSO OBSERVED: P=650D, P=3800D.
ST     AND    P VAR. MAX=2418370+337.3D*E (J.D.2418000-
              28000). OCE/SINCE J.D.2428000-CM.TA./
              SEE TABLE.
SU     AND    VB A (B 12.77M V, F0V:, 15").
SV     AND    BEHA MAX MEHETC EPOECK/THE MA-
              GNITUDE IN MAX VARIES PERIODICALLY, P=930D, P=
              5400D?  2146!.
SW     AND     FE/H!=+0.16. P VAR. HEHEH EH/NONLI-
              NEAR TERM:-1.229D*10**-10*E**2  1959!. OCE/SINCE
              1959 MAX=2436466.828+0.442270121D*E  6929!.
              OPMA KPBO ECKA MEHETC C -36.83D=
              83.28 P.  KOHEH (O-C) EMEHT -
              EKTA AKO MAX (O-C)=2436816.23+36.921D*N.
              BOMOH BEKOBO XO  KOEAH B (O-C) C
              EPOOM-2 OA  8005!./THE SHAPE OF THE
              LIGHT CURVE VARIES WITH -36.83D=83.28 P. THE
              DEVIATIONS (O-C) SATISFY THE ELEMENTS OF BLAZH-
              KO EFFECT MAX (O-C)=2436816.23+36.921D*N. SE-
              CULAR TREND AND CYCLIC (P-2A) VARIATIONS OF
              (O-C) ARE POSSIBLE  8005!.
SY     AND    D=0.027P.
TT     AND    MIN II 11.6?
TU     AND    P VAR (-37A?).
TV     AND    P VAR? DM CHO MEHETC./DM STRONGLY VARI-
              ES.
TW     AND    D=0.020P. MIN II 8.94. P VAR. MIN=2428845.422+
              4.122739D*E (J.D.2420050-32000). OCE/SINCE
              J.D.2432000-CM.TA./SEE TABLE.
TZ     AND    P1=118D:  0882!. CPEH BEHA MEHETC
              C/MEAN MAGNITUDE VARIES WITH P2=974D  0098!.
              P=135D (J.D.2437545-38377)  3367!.
UU     AND    P VAR. MIN=2428832.536+1.486311D E (J.D.
              2421455-23740)  2262!; MIN=2428832.465+
              1.48629D*E (J.D.2428830-35012)  0745!. OCE/
              SINCE J.D.2441100-CM.TA./SEE TABLE.
UW     AND    P VAR. O/BEFORE J.D.2430000 MAX=2418585+
              236.7D*E. OCE/SINCE J.D.2436000-CM.TA./
              SEE TABLE.
WW     AND    D=0.012P.
WX     AND    P VAR. MAX=2422613.614+3.0012544D*E
              (J.D.2422610-34712)  1240!. B TAE PBE-
              EH TEKE EMEHT. D=0.03P B 1972 , BO-
              MOHO, MEHETC./THE TABLE GIVES CURRENT ELE-
              MENTS. D=0.03P IN 1972 AND PROBABLY VARIES.
WZ     AND    MIN II 11.9. P VAR  2262!. MIN=2435075.342+
              +0.695662D*E (O/BEFORE J.D.2440500); BEPOTHO/
              PROBABLY MIN=2440872.290+0.6956576D*E OC-
              E/SINCE J.D.2440500. EMEHT B TAE
              OBETBOPTEHO PECTABT BCE HAE-
              H./THE ELEMENTS IN THE TABLE REPRESENT ALL
              THE OBSERVATIONS SATISFACTORILY.
XX     AND    P VAR. MAX=2418001.938+0.7227486D*E (1908-
              1932); MAX=2427106.403+0.7227591D*E (1932-
              1946)  2264!. OCE/SINCE 1946-CM.TA./
              SEE TABLE. DS=9. EKT AKO:/BLAZHKO EF-
              FECT: MAX=2437578+36D*N  3111!.
XY     AND    BOMOEH EKT AKO/BLAZHKO EFFECT IS PO-
              SSIBLE.
XZ     AND    MIN II 10.16; DII=0.26P. P VAR  2431, 6932, 8008,
              8593!. MIN=2432883.6046+1.3572708D*E (J.D.
              2431700-36150)  1977!; MIN=2441954.340+
              +1.357293D*E (OCE/SINCE J.D.2436200). EMEH-
              T B TAE OBETBOPTEHO PECTABT
              BCE HAEH./THE ELEMENTS IN THE TABLE REPRE-
              SENT ALL THE OBSERVATIONS SATISFACTORILY.
AA     AND    MIN II 10.5.
AB     AND    MIN II 10.20. P VAR. EPO PEKO BEC B
              1953 (-J.D.2434500)  C TEX OP OCTAETC O-
              CTOHHM  2509, 5222!/PERIOD INCREASED SUDDEN-
              LY IN 1953 (-J.D.2434500); NO PERIOD CHANGES
              LATER  2509, 5222!. EMEHT OCE/ELEMENTS SIN-
              CE 1953-CM.TA./SEE TABLE.
AC     AND    HEOHA MTEPOECKA EPEMEHHA./
              UNUSUAL MULTIPERIODICAL VARIABLE. BTOPOE KOEA-
              HE:/SECOND OSCILLATION: MAX=2432467.373+
              +0.71124243D*E; P3=0.421069D  8187!, CM.TAKE/
              SEE ALSO  8294, 8295!. DS=-1:.
AD     AND    MIN II 11.6. H MIN B ETX AX:/DEPTH
              OF MINIMA IN YELLOW LIGHT: 0.62M (MIN I), 0.58M
              (MIN II)  3141!. MIN II-MIN I=0.494P. P VAR. MIN=
              =2428718.402+0.9861940D*E (J.D.2417460-29640)
               1983!. OCE/SINCE J.D.2428700-CM.TA./
              SEE TABLE.
AE     AND    B AAKTKE M31./IN THE M31 GALAXY. CH
               KOHTHM./STRONG UV CONTINUUM. MCC/
              EMISSIONS H, HE I, FE II,  FE II!.
AF     AND    CM./SEE AE AND.
AG     AND    COACHO/ACCORDING TO  8296!, DSCT:, MIN=
              =2442636.5868+0.0347D E, A=0.5M.
AM     AND    VB A (B 0.25' S).
AN     AND    MIN II 6.09. B CCTEME BOMOHO HAE TPET-
              EO TEA./THE EXISTENCE OF THE THIRD BODY IN
              THE SYSTEM IS POSSIBLE. SP(MET)=F2-F5.
AP     AND    MIN II 11.9. BOMOHO, EPO CEET MEH-
              T BBOE./THE PERIOD MAY BE 2 TIMES SHORTER.
AT     AND    B-V: +0.42, +0.56. DS=3. MEHEH EPOA 
              OPOHOE CCEOBAHE CM.  8299!./SEE  8299!
              FOR DATA ON PERIOD VARIATIONS AND A DETAILED STU-
              DY.
BD     AND    MIN II 11.4.
BE     AND    CPEH K:/AVERAGE CYCLE: 137D  1993, 2267!;
              156.8D OCE/AFTER J.D.2431700.
BL     AND    HA/DEPTH OF MIN II 0.24M:. P VAR? MIN I=
              =2429491.255+0.7223779D*E (J.D.2415800-
              33900)  1995!. OCE/SINCE J.D.2433900-CM.
              TA./SEE TABLE.
BX     AND    ADS 1671 A (B 9.7M, 20", 59G). MIN II 9.15. BO-
              MOHO MEHEHE EPOA:/POSSIBLE PERIOD CHA-
              NGE: C/FROM 0.61011222D O/TO 0.61011534D
              (-1952). O MEHEHX EPOA CM.TAKE/
              ON THE PERIOD CHANGES SEE ALSO  8657!.
BY     AND    COACHO/ACCORDING TO  8658!, SRB:.
CC     AND    BOMOHO, B BOHO CCTEME C PORB=10.469D.
              AMTA  OPMA KPBO ECKA EPEMEHH
              C EPOOM 5.23714D  10.469D  8016!. COAC-
              HO  3120!, MEETC 4 EPOA: P2=0.0632083D.
              EPB OEPTOH HE HAEH. OCTAHE EPO-
              -PEOHAHCHE/POSSIBLY IN A BINARY WITH
              PORB=10.469D. DM AND THE LIGHT CURVE SHAPE VA-
              RY WITH A PERIOD 5.23714D OR 10.469D  8016!. ACCOR-
              DING TO  3120!, 4 PERIODS ARE PRESENT: P2=0.0632083D.
              FIRST OVERTONE WAS NOT FOUND. OTHER PERIODS ARE
              RESONANCES.
CG     AND    P VAR: 3.7430D (1950), 3.7394D (1963)  5224!. BO-
              MOH KECKE MEHEH EPOA. COAC-
              HO  6941!, METC KOPOTKOEPOECKE KO-
              EAH C EPOOM 2H04M. P HAATEE
              KABAET HA OTCTCTBE KOPOTKOEPOECKO
              EPEMEHHOCT./CYCLIC PERIOD CHANGES ARE POSSI-
              BLE. ACCORDING TO  6941!, SHORT PERIOD OSCILLATI-
              ONS (P=2H04M) ARE PRESENT. A NUMBER OF OBSER-
              VERS DO NOT FIND SHORT-TERM VARIABILITY.
CM     AND    COACHO/ACCORDING TO  0821!, MAX=2428380+
              +140D*E /AND MAX=2430616+124D*E,  BEA
              OXOA HA UU HER/AND THE STAR RESEMBLES UU
              HER.
CN     AND    MIN II 9.96.
CO     AND    D=0.06P:
CP     AND    D=0.01P? HA/DEPTH OF MIN II 0.05M?
CU     AND    D>0.034P ( 6943!, O BAHM HAEHM/
              ACCORDING TO VISUAL OBSERVATIONS).
DI     AND    DCEP?  3165!.
DK     AND    EW?
DL     AND    B OACT PACCEHHOO CKOEH/IN THE FIELD
              OF THE OPEN CLUSTER NGC 7686.
DR     AND    P VAR. O/BEFORE-J.D.2437000 MAX=2436078.384+
              +0.5630609D*E  2275!; ATEM P MEHC CKA-
              KOM/THEN P CHANGED ABRUPTLY. DM MEHETC HA/
              CHANGES BY-0.3M, MAX A1=2436078.8+69.486D*N1,
              MAX A2=2437646.65+69.719D*N2. BOMOH K-
               2000D (HTEPEPEH KOB N1  N2) -30
              ET  8019!./OTHER POSSIBLE CYCLES ARE 2000D (IN-
              TERACTION OF CYCLES N1 AND N2) AND-30 YEARS
               8019!.
DS     AND    B OACT PACCEHHOO CKOEH/IN THE FIELD
              OF THE OPEN CLUSTER NGC 752. MIN II 10.7.
DZ     AND    COACHO  4008!, T RCB, CEKTP R. COACHO
               6945!, C 1961 OCTOHHO HAXOTC B MAX. CO-
              ACHO  6946!, CEKTP HE XAPAKTEPEH  BE
              TA RCB. COACHO  8660!, A PKA B
              MOMEHTOB MIN, AHHX B  4008!./ACCORDING TO
               4008!, TYPE RCB, SPECTRUM R. ACCORDING TO  6945!,
              SINCE 1961 IS IN MAX LIGHT ALL THE TIME. ACCORDING
              TO  6946!, THE SPECTRUM IS NOT CHARACTERISTIC OF
              RCB STARS. ACCORDING TO  8660!, THE STAR WAS
              BRIGHT NEAR THE MOMENTS OF MIN LIGHT GIVEN IN
               4008!.
EG     AND    P=40D /OR 80D  8020!. HA CEKTP OOEH
              HAKABATC MCC BCOKOO BOEH
               4434, 8598!. CHOE EPEMEHHOE MAHTHOE
              OE  4435!. HAATC OOEPOECKE
              KOEAH ECKA. EBE CKOPOCT, PO 
              KBBAEHTHE PH H MEHTC C P=470D
               8596! (SB?  8597!). BOMOHO, CXOHA C HM
              SGE  8598!./ABSORPTION SPECTRUM WITH OVERLAYING
              EMISSIONS OF HIGH EXCITATION  4434, 8598!. STRONG
              VARIABLE MAGNETIC FIELD  4435!. LONG PERIOD VARIA-
              TIONS OF LIGHT ARE OBSERVED. RADIAL VELOCITIES PRO-
              FILES AND EQUIVALENT WIDTHS OF LINES VARY WITH P=
              =470D  8596! (SB?  8597!). POSSIBLY IS ANALOGO-
              US TO HM SGE  8598!.
EH     AND    K TOK. BOMOHO HAE EBO OOO-
              K./IR EXCESS. THE PRESENCE OF A DUST ENVELOPE IS POSSIBLE.
EO     AND    OEH KPACHA./VERY RED.
EP     AND    MIN II 12.5.
ET     AND    DB=0.035M, DU=0.07M. B TAE AHA OXA MAX
              ECKA. EPO 0.723D  1.61553D OBETBOP-
              T HAEHM  8022, 7946!. COACHO  8023!,
              B HE-EKAPE 1977 MIN=2443337.4725+
              +0.49925D*E, PE EPO HAEHM HE
              OBETBOPT. COACHO  8599!, MAX(U)=
              =2439751.28+0.617135D*E (1967-1971). SB,
              MAX(VR)=J.D.2443718.0+48.304D*E  8301!. O-
              TOMETPECKE EPO B EBX CKOPOCTX
              HE HAEH./THE TABLE GIVES THE EPOCH OF MAX
              LIGHT. OBSERVATIONS MAY BE REPRESENTED BY THE PE-
              RIODS 0.723D AND 1.61553D  8022, 7946!. ACCORDING
              TO  8023!, IN JUNE-DECEMBER 1977 MIN=
              =2443337.4725+0.49925D*E, OTHER PERIODS ARE
              NOT SATISFIED BY OBSERVATIONS. ACCORDING TO  8599!,
              MAX(U)=2439751.28+0.617135D*E (1967-1971).
              SB, MAX(VR)=J.D.2443718.0+48.304D*E  8301!.
              PHOTOMETRIC PERIODS COULD NOT BE FOUND IN RADI-
              AL VELOCITIES.
EX     AND    BOMOEH/POSSIBLE MIN II 13, 0:, MIN II-MIN I=
              =0.55P.
EY     AND    I-K=5.38; BOMOHO HAE EBO OOOK/
              THE PRESENCE OF A DUST ENVELOPE IS POSSIBLE
               6947!.
FF     AND    10.35M-10.42M V BHE BCEK/OUTSIDE FLARES;
              M-M=0.50P. PORB=2.170304D  8024!. O OTOMET-
              PECKM HAEHM/ACCORDING TO PHOTOMET-
              RIC OBSERVATIONS P=2.14D (1971), P=2.15D (1972),
              P=2.19D (1973)  6948!.
FG     AND    COACHO/ACCORDING TO  4156!, EA; MIN=
              =2436074.528+0.99772D*E.
FL     AND    D=0.02P.
FZ     AND    MU=1", P=64G.
GK     AND    MIN II 11.5.
GN     AND    ADS 409 A (B 13.3M, 2", 6G; C 11.6M, 141", 130G).
              PAHE ABTOP AT CEKTP F0 III, F2V, AM
              (O-BMOM, O PAHM KPTEPM)./DIFFERENT
              AUTHORS GIVE SPECTRAL TYPES F0 III, F2V, AM (PRO-
              BABLY BASED ON DIFFERENT CRITERIA).
GP     AND    DM MEHETC C P2=0.64D. AMETHA BOHA C P3=
              =0.012161D. CPEH BEHA  KPBA ECKA
              MEHTC  8302!./DM CHANGES WITH P2=0.64D.
              A WAVE WITH P3=0.012161D IS PRESENT. THE MEAN
              MAGNITUDE AND THE SHAPE OF THE LIGHT CURVE VARY
               8302!.
GQ     AND    ADS 246 B (A=GX AND; B 37", 61G). B-V=+1.80.
              CTOHK PEHTEHOBCKOO EH/X-RAY SOU-
              RCE.
GR     AND    MIN (MAH.OE/MAGNET.FIELD)=2442288+525D*E.
              MAHTHOE OE MEHETC OT-250 O-1030 ACC.
              EPO MEHEH C1 OKOO 1.5 ET  7893!.
              COACHO  6257! EPO MEHEH B U OKOO
              1 OA  OEE./MAGNETIC FIELD VARIES (-250
              TO-1030 GAUSS). PERIOD OF CHANGES OF C1 IS NE-
              AR 1.5 YEARS  7893!. ACCORDING TO  6257!, PERIOD
              OF CHANGES IN U IS NEAR 1 YEAR OR LONGER.
GS     AND    B-V=+1.7 B HOPMAHOM ECKE/IN NORMAL
              LIGHT.
GX     AND    ADS 246 A (B=GQ AND, 37", 61G). DU=0.55M. SB?
              (AHHE POTBOPEB/CONFLICTING DATA).
GY     AND    SB 1 (P=273.2D  7324!, P=272.99D  8303!). 
              CEKTPAHX MEHEH, MEHEH BETA 
              MAHTHOO O BOMOEH P=23A  7004! 
              20.60A  8303!. B  8022! AETC P-36.5D  DV=
              =0.049M. BOMOHO, METC EPO 4.92A 
              1.8D  8303!./FOR SPECTRAL CHANGES, VARIATIONS OF
              LIGHT AND MAGNETIC FIELD IT IS POSSIBLE THAT P=
              =23A  7004! OR 20.60A  8303!.  8022! GIVES P-36.5D
              AND DV=0.049M. PERIODS 4.92A AND 1.8D MAY EXIST
               8303!.
GZ     AND    B-V:+0.77, +0.82. ADS 1693 A (B 11.13M, 8", 31G).
              MIN II 11.58. P VAR.? EPO OPEEEH TOKO
              O MIN I  6830!  TOHEH O OCEHM OXAM.
              /THE PERIOD IS BASED ONLY ON MINIMA I  6830! AND
              WAS IMPROVED WITH ACCOUNT OF RECENT DATA.
HH     AND    CKAPK?/SUBDWARF?  6581!. MU=1.82", P=176G.
HI     AND    B-V=1.8M BHE BCK/OUTSIDE FLARES.
HN     AND    MAX(U)=2438327.8+69.433D*E  8022!. SB
              (P=106.27D  7435!).
HQ     AND    COACHO  8659!, BEPOTHA KATAKMECKA
              BOHA CCTEMA; OTMEAETC CXOCTBO C AM
              HER  AN UMA./ACCORDING TO  8659!, A PROBABLY
              CATACLYSMIC BINARY; SIMILARITY TO AM HER AND AN
              UMA IS NOTED.
HR     AND    D=0.05P.
HT     AND    B-V=+0.60. B OACT/IN THE REGION OF M 31.
HU     AND    MIN II 17.2. B OACT/IN THE REGION OF M 31.
HV     AND    CM./SEE HQ AND.
HY     AND    B OACT/IN THE REGION OF M 31.
HZ     AND    CM./SEE HY AND. P>100D. KPACHA/RED.
IL     AND    D=0.02P.
IM     AND    CM./SEE HY AND. MIN II 18.8.
IO     AND    CM./SEE HQ AND.
IP     AND    D=0.02P:.
KK     AND    KPBA ECKA MEET B BOHO BOH  7740!.
              OTMEEH OOEPOECKE KOEAH
               7955!./THE LIGHT CURVE HAS DOUBLE-WAVE SHAPE
               7740!. LONG PERIOD VARIATIONS WERE FOUND  7955!.
KU     AND    I-K=4.63. BOMOEH T SR. OKPEHA E-
              BO OOOKO  8029!./SR TYPE IS POSSIBLE. SUR-
              ROUNDED WITH A DUST ENVELOPE  8029!.
KX     AND    SB 2 (P=38.908D).
KZ     AND    ADS 16557 B (A 7.0M; B 15", 254).
LM     AND    MIN II 12.7.
LN     AND    DB=0.025.
LO     AND    MIN II 11.82.
ALFA   AND    SB (P=96.6960D). VB A (B 11.2M, 80"). PBEEHA
              OXA MAX ECKA B CCTEME U. HEKC HBETA ME-
              HETC C AMTO-0.02M  P-3H  8030!. -
              CTPOE BPAEHE./EPOCH OF MAX U LIGHT IS GIVEN.
              HBETA INDEX VARIES IN THE RANGE OF-0.02M WITH P
              -3H  8030!. RAPID ROTATION.
       AND    HA/DEPTH OF MIN II 0.1M. SB. KPBA EC-
              KA HECTAHA. HAOE BAPA HA BOCXO-
              E BETB MAX II  8030!. MHOO OCOEHHOCTE
              B CEKTPE./UNSTABLE LIGHT CURVE. MOST NOTABLE
              VARIATIONS ON THE RISING BRANCH OF MAX II  8030!.
              MANY PECULIARITIES IN THE SPECTRUM.
LAMBDA AND    SB 1 (P=20.52D).
OMIKRO AND    V SIN I=300 KM/S; VB(0.3"; BOMOHO TAKE/PO-
              SSIBLY ALSO 0.05"-O CEK-HTEPEPOMETP
              /ACCORDING TO SPECKLE-INTERFEROMETRIC DATA). C
              1890  BE HECKOKO PA OBC  CE-
              A CEKTP OOOK. HEOHOKPATHO OTHOCAC
              PAHM ABTOPAM K EPEMEHHM TA EB.
              COACHO  5955!, BOMOHO TAKE, TO MEHE-
              H ECKA O'CHTC ECKM MEHEHM
              OHOHO BE C OOOKO. OH PECTABTC
              EMEHTAM MIN I=2439470.628+1.0185D*E. CO-
              ACHO  2572!, MIN I=2436174.430+1.5998398D*E.
              EPOOPAMMH AHA HAEH OKABA-
              ET CTOB K P P-0.84D  8032!. B KOHE
              1975, BOMOHO, POOE CPOC OOOK.
              /SHELL SPECTRUM APPEARED AND DISAPPEARED SEVE-
              RAL TIMES SINCE 1890. DIFFERENT AUTHORS ATTRIBUTED
              THE STAR TO EB TYPE. ACCORDING TO  5955!, THE CHAN-
              GES OF LIGHT MAY BE EXPLAINED ALSO BY INTRINSIC
              VARIATIONS OF A SINGLE SHELL STAR. THEY ARE REPRE-
              SENTED BY ELEMENTS: MIN I=2439470.628+1.0185D*E.
              ACCORDING TO  2572!, MIN I=2436174.430+
              +1.5998398D*E. THE PERIODOGRAM ANALYSIS SHOWS
              A STABLE PEAK AT P-0.84P  8032!. A POSSIBLE SHELL
              EVENT WAS OBSERVED LATE IN 1975.
S      ANT    MIN II 6.87. P VAR?
T      ANT    CWB? P VAR.  A/H!=-0.0. P=5.9098D (J.D.2428187-
              34688), P=5.8976D (J.D.2434688-37660)  5387!.
              B TAE-CPEHE EMEHT, CPABHTEHO
              XOPOO OBETBOPE BCEM HAEHM.
              /THE TABLE GIVES MEAN ELEMENTS WHICH SATISFY
              ALL OBSERVATIONS WELL ENOUGH.
V      ANT    MAEP/OH, H2O MASER.
Z      ANT    CPEH ECK MEHETC C/MEAN BRIGHTNESS VA-
              RIES WITH P=1143D.
SW     ANT    MIN II 14.6.
UZ     ANT    P VAR?
WY     ANT    P VAR. P=0.57430871D (J.D.2414000-22070); P=
              =0.57431618D (J.D.2422070-25600); P=0.57431216D
              (J.D.2425600-29000)  1113!. (K-B)2=0.00.
WZ     ANT    MIN II 11.8.
XX     ANT    MIN II 9.1.
XY     ANT    HA/DEPTH OF MIN II 0.3M-0.5M PG.
XZ     ANT    MIN II 10.2.
Z      APS    BOMOHO, BETC TAKE ATMEHHO/POSSIB-
              LY ALSO AN ECLIPSING BINARY.
RT     APS    EPO  OPMA KPBO ECKA CHO MEHT-
              C/STRONG VARIATIONS OF PERIOD AND THE SHAPE OF
              THE LIGHT CURVE  6152!.
TY     APS    DS=3.
YY     APS    EPO, BEPOTHO, OO/THE PERIOD IS PRO-
              BABLY LONG.
AF     APS    MIN II 13.9.
AN     APS    MIN II 12.8.
AP     APS    MIN II 15.5.
AS     APS    MIN II 13.8.
AV     APS    HA/DEPTH OF MIN II 0.05M.
CE     APS    P=209D /OR 261D.
CY     APS    MIN II 13.0.
EF     APS    MIN II 12.6.
FY     APS    OK/DEEP MIN II.
GK     APS    MIN II 13.9. BOMOEH T RRC/RRC TYPE IS PO-
              SSIBLE.
GO     APS    MIN II 14.8. BOMOEH T RR/RR TYPE IS POSSI-
              BLE.
GQ     APS    MIN II 14.8.
GU     APS    MIN II 14.5.
GX     APS    HE CKEH T RV. AHA OXA MIN/RV TYPE
              IS NOT EXCLUDED. THE EPOCH OF MIN IS GIVEN.
GY     APS    MIN II 14.2.
HL     APS    MIN II 12.6.
HO     APS    MIN II 13.7.
HT     APS    MIN II 14.3.
HV     APS    AHA OXA MIN/EPOCH OF MIN IS GIVEN.
HX     APS    MIN II 14.4.
II     APS    MIN II 11.6.
IL     APS    CM./SEE HV APS.
IO     APS    MIN II 12.4.
IR     APS    MIN II 13.8.
IU     APS    MIN II 14.6.
IY     APS    MIN II 12.9.
KN     APS    D-0.03P.
KR     APS    BOMOHO, MEEHHA ATMEHHA/POSSIBLY A
              SLOW ECLIPSING VARIABLE.
KT     APS    MIN II 15.2.
KV     APS    MIN II 13.6.
KZ     APS    HA ABHE KOEAH ECKA HAKABATC
              KOEAH ATMEHHOO XAPAKTEPA C MHM-
              MAM B J.D.2436729  2436808/SMOOTH LIGHT
              CHANGES WITH SUPERIMPOSED VARIATIONS OF ECLIP-
              SING NATURE, WITH MINIMA ON J.D.2436729 AND
              2436808.
LM     APS    BOMOEH T RV/RV TYPE IS POSSIBLE.
LN     APS    MIN II 13.3.
LO     APS    MIN II 11.5.
MY     APS    L19-2. P0=192.75S, P1=113.77S.
DELTA* *1     APS B POKO APE/IN A WIDE PAIR (DELTA**2 APS, 100",
              OEE/COMMON MU).
KAPPA* *1     APS SB? VB A (B 11.27M V, 27").
R      AQR    CEKTP KOMHPOBAHH. MCC H, SII, OIII,
              FE II, NE III, OII. EPEMEHHOE PAOEHE.
              MAEP SIO. BOMOHO, BTOPO KOMOHEHT B-
              ETC AKKPEPM EM KAPKOM. BEA
              OPEHA B PACPC AOB TMAH-
              HOCT C BOPACTOM B HECKOKO CTOET. B -
              MEHEHX EBX CKOPOCTE  EPOA BOMO-
              EH K-24A  OEE OOEPOECKE KO-
              EAH  8055!./SYMBIOTIC SPECTRUM. EMISSIONS
              OF H, SII, OIII, FEII, NEIII, OII. VARIABLE RADIO SOUR-
              CE. SIO MASER. THE SECONDARY MAY BE AN ACCRE-
              TING WHITE DWARF. THE STAR IS EMBEDDED IN AN EX-
              PANDING GASEOUS NEBULA SEVERAL HUNDRED YEARS
              OLD. A CYCLE-24A AND LONGER-TERM VARIATIONS ARE
              POSSIBLE IN THE CHANGES OF RADIAL VELOCITIES AND
              PERIOD.
U      AQR    B CEKTPE CHE OOC 12C2, CN, H
              SRII, YII, ET BOOPOA. BEPOTHA BEA
              AO (VR-100 KM/C)./STRONG BANDS OF 12C2, CN,
              LINES OF SRII, YII IN THE SPECTRUM; HYDROGEN DEFICI-
              ENCY. A PROBABLE HALO STAR (VR-100 KM/S.).
Z      AQR    1969-70: P=100D+- 5973!.
RY     AQR    P VAR. MIN=2433872.352+1.966598D*E (O/BEFORE
              J.D.2428000); MIN=2440824.410+1.966620D*E
              (J.D.2428000-41000); MIN=2440824.410+
              +1.966611D*E (J.D.2441000-43800). OCE/SINCE
              J.D.2443800 P=1.966554D? EMEHT B TAE
              PECTABT HAEH C J.D.2428000 C TO-
              HOCT +-0.1D/THE TABLE GIVES ELEMENTS REPRESEN-
              TING OBSERVATIONS AFTER J.D.2428000 WITH THE ACCU-
              RACY +-0.1D.
ST     AQR    MIN II 9.37. P VAR. MIN=2423640.271+0.78101367D*E
              (J.D.2423500-26000)  2037!. OCE/SINCE
              J.D.2439700-CM.TA./SEE TABLE.
SU     AQR    ADS 16318 A (B 10.7M, 5", 144G). MIN II 10.5. P VAR?
SV     AQR    K/CYCLE 200-300D BOMOEH/IS POSSIBLE.
SW     AQR    P VAR. (K-B)2=0.01.
SX     AQR    P VAR? DS=9.
SZ     AQR    AHA OXA MIN/EPOCH OF MIN IS GIVEN.
TT     AQR    VB A (B 15M, 3", 135G).
TZ     AQR    DS=5.
VY     AQR    BTOPA BCKA/SECOND OUTBURST: MAX-J.D.2437897
              (1962), -9M PG  3129!.
WX     AQR    BOMOEH EKT AKO/BLAZHKO EFFECT IS POS-
              SIBLE.
XZ     AQR    P VAR. O/BEFORE J.D.2437913 P=2.059187D.
YZ     AQR    B-V=0.49 (B/IN MIN). (K-B)2=0.06. BOMOH
              HEOE KTA EPOA/SMALL FLUCTUATI-
              ONS OF PERIOD ARE POSSIBLE.
AE     AQR    HEOHA BCXBAA PEHTEHOBCKA CCTEMA
              C CAPOM. B MIN B-V=+0.92. B MAX OEET.
              KOEAH ECKA CTPE  HEPABHE, EM
              OHA OTAETC OT EPEMEHHX TA UV CET 
              CCTEM TA UG, XOT CEKTP MET OPEE-
              EHHOE CXOCTBO. OHOBPEMEHHE OTOEKTP-
              ECKE  CEKTPAHE HAEH  3131! O-
              KAA HAE BX BOB BCEK: 1) CEHE
              MCCOHHX H, COPOBOAEMOE BEE-
              HEM ECKA B U  B; 2) CEHE KOHTHMA,
              OTPAAEEC HA BEEH ECKA B OACTX
              U, B  V ("EA BCKA"). OPOHOE CCE-
              OBAHE CEKTPA  1971!. PORB=0.41165794D+
              +1.12D*10**-10*E, OXA T0=J.D.2439030.621
               8672!. B PEHTEHOBCKOM AAOHE (0.1-4.0 KEV)
              HAATC CA C P=33.0767S  8673!.
              B OTECKOM AAOHE-CA C P0=
              =33.076737S  C P1=16.5S  8674, 8675!./ UNUSU-
              AL FLARE X-RAY SYSTEM WITH PULSAR. BECOMES BLUER
              IN MAX. IN MIN B-V=+0.92. SHOWS RAPID IRREGULAR
              VARIATIONS, WHICH DIFFERS IT FROM UV STARS AND UG
              SYSTEM, THOUGH THE SPECTRA ARE SOMEWHAT SIMILAR.
              SIMULTANEOUS PHOTOELECTRIC AND SPECTROSCOPIC OB-
              SERVATIONS  3131! SHOW THE EXISTENCE OF TWO TYPES
              OF FLARES: 1) INTENSIFICATION OF EMISSION LINES AC-
              COMPANIED BY BRIGHTENING IN U AND B; 2) INTENSIFI-
              CATION OF CONTINUUM LEADING TO BRIGHTENING IN U,
              B AND V ("WHITE FLARE"). DETAILED SPECTROSCOPIC
              INVESTIGATION  1971!. PORB=0.41165794D+
              +1.12*10**-10*E, THE EPOCH T0=J.D.2439030.621
               8672!. IN THE X-RAY BAND (0.1-4.0 KEV) PULSATI-
              ONS WITH P=33.0767S ARE OBSERVED  8673!. IN THE
              OPTICAL RANGE PULSATIONS WITH P0=33.076737S AS
              WELL AS WITH P1=16.5S WERE NOTED  8674, 8675!.
AT     AQR    MIN II 14.7.
AX     AQR    P VAR. O/BEFORE-J.D.2427367 MAX=
              =2425417.60+0.388135D*E  3113!.
AY     AQR    MIN II 14.3.
BH     AQR    P VAR. O/BEFORE-J.D.2431150 MAX=2426948.411+
              +0.5258022D*E  3113!.
BI     AQR    MIN II 13.1.
BK     AQR    TECH CTHK/CLOSE COMPANION.
BL     AQR    BOH OT 80 O 125D. CPEH ECK MEHETC
              BOHAM OT 480 O 700D C AMTO 0.3M-0.6M.
              /WAVES FROM 80 TO 125D. MEAN MAGNITUDE CHANGES
              WITH CYCLES FROM 480 TO 700D IN THE RANGE OF 0.3M-
              0.6M.
BM     AQR    CPEH BEHA, BOMOHO, MEHETC C P=
              =500-600D./THE MEAN MAGNITUDE MAY VARY WITH
              P=500-600D.
BN     AQR    DS=4:. P VAR. O/BEFORE J.D.2428964 MAX=
              =2426577.901+0.46963401D*E  3113!. COACHO
              /ACCORDING TO  5391! MAX=2429395.742+
              +0.4696410D*E+3.3*10**-10*E**2 (1898-1958).
BO     AQR    P VAR? (K-B)2=0.01.
BQ     AQR    D=0.07P.
BR     AQR    P VAR? (K-B)2=0.16.
BS     AQR    DS=0. P VAR?
BT     AQR    B-V:+0.14, +0.52. P VAR. EKT AKO.
              /BLAZHKO EFFECT.
BV     AQR    P VAR. EKT AKO C =11.56D  KOEAHM
              ECKA B MAX O 0.75A./BLAZHKO EFFECT WITH =
              =11.56D AND VARIATIONS OF LIGHT IN MAX UP TO 0.75A.
BW     AQR    D=0.01P. MIN II 10.8. MIN II-MIN I=0.484P. EH
               0189! CTAET BTOPH MIN ABHM./JENSCH
               0189! CONSIDERS THE SECONDARY MIN TO BE THE
              MAIN ONE.
BX     AQR    D=0.027P.
CD     AQR    D=0.012P. MIN II 10.2.
CE     AQR    COACHO  2548!, BAHE HAEH B TE-
              EHE PA MECEB B 1954-1958 HE OKAA
              EPEMEHHOCT. O AHHM  3138!, BOMOHO, O-
              OHA AI VEL; P=0.16D?/ACCORDING TO  2548!, NO
              VARIATIONS WERE FOUND IN VISUAL OBSERVATIONS DU-
              RING SEVERAL MONTHS IN 1954-1958. ACCORDING TO
               3138!, THE STAR MAY BE ANALOGOUS TO AI VEL; P=
              =0.16D?
CH     AQR    P VAR?
CI     AQR    EPO, BOMOHO, HAO BOT/PERIOD MAY
              BE TWICE AS LONG.
CM     AQR    MIN II 13.6.
CP     AQR    DS=3.
CR     AQR    MIN II 14.2.
CV     AQR    AHHE   6072! HE ACBAT OBEP./DATA
              IN  6072! ARE NOT RELIABLE.
CW     AQR    MIN II 10.8.
CX     AQR    MIN II 10.8. H BOOPOA POKE./BROAD HYD-
              ROGEN LINES.
CY     AQR    DS=2. P VAR; CKAKOOPAHOE MEHEHE/ABRUPT
              CHANGE-1952. O/BEFORE J.D.2434000 MAX=
              =2434308.4314+0.061038509D*E. OPMA KPBO
              ECKA, O-BMOM, MEHETC.  M-M PAHE
              ABTOP AT HAEH OT 0.23P O 0.40P. BOMO-
              H EH C P2=0.2182D  8060!./THE SHAPE OF
              THE LIGHT CURVE PROBABLY VARIES. FOR M-M DIFFE-
              RENT AUTHORS GIVE VALUES FROM 0.23P TO 0.40P. BEAT
              PHENOMENON WITH P2=0.2182D IS POSSIBLE  8060!.
CZ     AQR    MIN II 11.1. KECKE MEHEH EPOA?
              /CYCLIC VARIATIONS OF PERIOD?
DD     AQR    MIN II 11.2.
DN     AQR    (K-B)2=0.01.
DO     AQR    P VAR.
DS     AQR    P VAR.
DV     AQR    MIN II 6.1. SB. B  8061! OTMEEH MEHEH C
              DM-0.1M  P<3H, CBBAEME C EPEMEHHOCT
              TA DSCT. O HEKOTOPM CTOHKAM CEKTP
              A 3. B MAE 1975 HAAC CEKTP OOOK:
              CEKTPAHE H AT MCCE  CA;
              CHOE OOEHE B HX H  K CA II. B
              CEKTPAX 1971-1973 EKT OOOK OTCT-
              CTBT  8062!./IN  8061! VARIATIONS WERE NOTED
              WITH DM-0.1M AND P<3H, PRESUMABLY OF DSCT
              TYPE NATURE. SOME SOURCES GIVE A 3 FOR THE SPECT-
              RAL TYPE. SHELL SPECTRUM WAS OBSERVED IN MAY,
              1975. SPECTRAL LINES WERE FILLED WITH EMISSION
              AND THEREFORE WEAK, STRONG ABSORPTION IN H AND
              K CAII LINES WAS PRESENT. SHELL EFFECTS WERE NOT
              PRESENT IN THE SPECTRA TAKEN IN 1971-1973  8062!.
DX     AQR    VB B (A 7.0M, K0 III; B 3.7", 244G). SB 1. D-0.015P.
              HA/DEPTH OF MIN II-0.3M. AH PEE
              MEHEH CMMAPHOO ECKA./THE RANGE OF
              COMBINED BRIGHTNESS IS GIVEN.
DY     AQR    D=0.04P.
EE     AQR    MIN II 8.48.
EK     AQR    MIN II 11.23.
EL     AQR    P=0.6345D BOMOEH/IS POSSIBLE.
EM     AQR    COACHO/ACCORDING TO  6204! P=0.068D. EPO
               AMTA MEHTC A OEH KOPOTKOE BPEM.
              ECK  BET MEHTC PMEPHO B AE. EC
              CECTBET EPO EH, TO OH MEHE 1D.
              /PERIOD AND AMPLITUDE VARY ON VERY SHORT TIME
              SCALE. LIGHT AND COLOUR VARY APPROXIMATELY IN PHA-
              SE. THE BEAT PERIOD, IF EXISTS, IS SHORTER THAN 1D.
ET     AQR    EPO AH COACHO  8336!./PERIOD IS GIVEN AC-
              CORDING TO  8336!.
EW     AQR    DM EPEMEHHA/VARIES.
FF     AQR    D=0.059P. SB 1. HKAHA ATMEHHA CCTEMA
               KPACHO BE , BEPOTHO, OOO OPE-
              O CKAPKA. AMTA ATMEH 0.15 V,
              0.4 B, 1.2 U. ECK B MAKCMME MEHETC HA
              0.35V, 0.33B, 0.22U. OPMA KPBO ECKA E-
              PEMEHHA. B CEKTPE-CHE MCC H 
              K CA II, HALFA./THE UNIQUE ECLIPSING SYSTEM OF A
              RED STAR AND PROBABLY A BLUE HOT SUBDWARF. THE AM-
              PLITUDE OF THE ECLIPSE IS 0.15V, 0.4B, 1.2U. THE
              MAGNITUDE IN MAX VARIES BY 0.35V, 0.33B, 0, 22U.
              VARIABLE SHAPE OF LIGHT CURVE. STRONG EMISSIONS H
              AND K CAII, HALFA IN THE SPECTRUM.
FI     AQR    BOMOHO/POSSIBLY P=4.659D /OR 4.719D. P-
              BEEHA OXA MIN/EPOCH OF MIN IS GIVEN.
FK     AQR    BDS 11854 A(B=FL AQR, 11.45M, 24", 352G, 1966).
              MU ALFA=+0.455", MU DELTA=-0.067". SB 2 (P=4.08322D       .
 0313!)
              BCK/FLARES DU=0.7  0344!.
FL     AQR    BDS 11854 B (A=FK AQR; B 24", 352G, 1966).
OMIKRO AQR    HAAETC CEKTP OOOK  CKA./SHELL
              OR DISK SPECTRUM IS OBSERVED.
PI     AQR    B 1957-1975 ECK BOPOC HA-0.2M V, BEA O-
              KPACHEA. MCCOHH AMEPOBCK KOHTHM.
              CTPE MEHEH B MCCOHHX HX  B
              OPA. BOMOHO, BEA MEET CK 
              OOOK./THE BRIGHTNESS INCREASED BY-0.2M V
              IN 1957-1975, THE STAR BECAME REDDER. BALMER
              CONTINUUM IN EMISSION. RAPID CHANGES IN EMISSI-
              ON LINES AND IN POLARIZATION. EXISTENCE OF A DISK
              OR A SHELL IS POSSIBLE.
R      AQL    P VAR. MAX=2440038+297D. E (J.D.2427850-40000).
              OCE/SINCE J.D.2440000-CM.TA./SEE TABLE.
              HA BCEM HTEPBAE HAEH/FOR THE WHOLE OBSER-
              VED PERIOD MAX=2399190+346.932D*N-0.239303D*N**2;
              PN=348.980D-0.554202D*N+0.000552309D*N**2  3143!.
              H2O-, OH-,  SIO-MAEP. PAOBCK./H2O,
              OH AND SIO MASER. RADIOBURSTS.
U      AQL    B-V:+0.84, +1.24. P VAR. ADS 12503 A (B 14.00M,
              35", 349G, 1900; EE OH CTHK/ONE MORE COMPA-
              NION 11.7M V, 2", 230G, 1934).
W      AQL    S 6/6E. B MIN CEKTP COCTABHO; BOMOHO,
              MEETC CTHK CO CEKTPOM F5-F8  3502!./
              COMPOSITE SPECTRUM NEAR MIN LIGHT; A COMPANION
              (F5-F8) MAY EXIST  3502!.
Y      AQL    HA/DEPTH OF MIN II 0.03M. SB 1.
RR     AQL    MAEP/MASER H2O, OH, SIO.
RT     AQL    CM./SEE RR AQL.
SY     AQL    MAEP/MASER H2O, OH.
SZ     AQL    B-V:+1.04, +1.82. P VAR  2392!. O/BEFORE
              J.D.2420260 P=17.1359D. TEKE EMEHT
              /CURRENT ELEMENTS-CM.TA./SEE TABLE.
TT     AQL    B-V:+0.96, +1.62. P VAR.  2392!. O/BEFORE
              J.D.2418035 P=13.7518D. TEKE EMEHT/
              CURRENT ELEMENTS-CM.TA./SEE TABLE.
TV     AQL    P VAR (MEHC/CHANGED AT-J.D.2430000). O
              /BEFORE J.D.2430000 MAX=2429730+237.9D*E.
TW     AQL    B PAHE HTEPBA BPEMEH HAATC
              K 65D  95D  8714!./CYCLES 65D OR 95D ARE
              OBSERVED DURING DIFFERENT TIME INTERVALS  8714!.
UU     AQL    CPEH K/MEAN CYCLE: 71.3D  4063!; 56D
               3144!.
UY     AQL    B  0504! OTMEEH KECKE MEHEH
              ECKA (P-400D), HA KOTOPE HAKABATC
              OEH CTPE KOEAH./CYCLIC CHANGES OF
              LIGHT (P-400D) WITH SUPERIMPOSED VERY RAPID VA-
              RIATIONS ARE NOTED IN  0504!.
VX     AQL    SC 5-/8E. COACHO  4231!, HEPABHA. -
              TEBA BEA./ACCORDING TO  4231!, THE VARIA-
              BLE IS IRREGULAR. LITHIUM STAR.
VZ     AQL    B-V:+0.61, +1.01.
XZ     AQL    P VAR. MIN=2424449.277+2.139147D*E
              (J.D.2424380-2430300). OCE/SINCE
              J.D.2433000-CM.TA./SEE TABLE.
YZ     AQL    D=0.03P. P VAR.
AA     AQL    DS=1.0.
AC     AQL    P VAR.
AD     AQL    B CEKTPE HAATC OOC CN. COACHO
               6928!, PEE 8.83-13.42 V./CN BANDS ARE
              OBSERVED IN THE SPECTRUM. ACCORDING TO  6928!,
              THE RANGE IS 8.83-13.42 V.
AE     AQL    VB A (B 16.6M, 12", 330G; C 16.9M, 11", 0G). CM-
              MAPH ECK MEHETC B PEEAX 13.9-15.8.
              /THE COMBINED LIGHT OF A, B, C VARIES IN THE RAN-
              GE 13.9-15.8.
AF     AQL    BOMOHO, EPO BBOE MEHE./THE PERIOD
              MAY BE TWO TIMES SHORTER.
AL     AQL    D=0.04P.
AU     AQL    COACHO/ACCORDING TO  3146!, P=190D /OR
              380D.
BL     AQL    P VAR. MAX=2418538+159.65D*E (J.D.2418529-
              -29075). B HTEPBAE/DURING J.D.2436420-
              -38940-CM.TA./SEE TABLE.
BY     AQL    P VAR?
CD     AQL    TECH CTHK?/CLOSE COMPANION?
CL     AQL    HOA PECKABAEME O EMEHTAM MAKC-
              MM HE HACTAT./SOMETIMES MAXIMA PREDIC-
              TED ACCORDING TO THE ELEMENTS DO NOT OCCUR.
CM     AQL    CEKTP KOMHPOBAHH, CXOEH CO CEKTPOM
              Z AND  3149!./SYMBIOTIC SPECTRUM SIMILAR TO
              THAT OF Z AND  3149!.
CR     AQL    BOMOEH HATEH EKT AKO./CON-
              SIDERABLE BLAZHKO EFFECT IS POSSIBLE.
CS     AQL    CM./SEE CD AQL.
CT     AQL    COACHO  6004!, B 1963-1968 HAAC
               MEEHHE HEPABHE KOEAH EC-
              KA C DM-0.6./ACCORDING TO  6004!, ONLY SLOW
              IRREGULAR VARIATIONS WITH DM-0.6 WERE OBSERVED
              IN 1963-1968.
CU     AQL    P VAR? (BOMOHOE MEHEHE/POSSIBLE CHANGE
              -J.D.2423000). O TOO/EARLIER MAX=2418591+
              +203.7D*E.
CV     AQL    P VAR?
CW     AQL    CM./SEE CD AQL.
DD     AQL    CM./SEE CD AQL.
DT     AQL    P VAR (MEHEHE/CHANGE-J.D.2425000). O TO-
              O/EARLIER MAX=2423964+290.5D*E.
DY     AQL    P VAR  6107!.
EV     AQL    P VAR. O/BEFORE J.D.2423900 P=38.67D.
               A/H!=-0.3.
EX     AQL    HAAETC TAKE P=117D./P=117D IS ALSO
              OBSERVED.
EZ     AQL    P VAR  6107!.
FF     AQL    ADS 11884 A (B 10.37M, 7", 141G). SB 1 (P=1435D).
FG     AQL    HA KPA TEMHO TMAHHOCT BARNARD 130. BO-
              MOHO, ECK CTHK FH AQL (RO-20").
              COACHO  0504!, CPEH K MEHEH EC-
              KA 3.5D. CPEH ECK MEHETC./AT THE EDGE
              OF THE DARK NEBULA BARNARD 130. MAY BE A PHYSI-
              CAL PAIR WITH FH AQL (RO-20"). ACCORDING TO
               0504!, THE MEAN CYCLE OF LIGHT VARIATIONS IS 3.5D.
              THE LEVEL OF MEAN LIGHT VARIES.
FH     AQL    O OOEH  BOCTBEHHOCT CM. FG AQL./ON
              THE POSITION AND BINARITY SEE FG AQL. COACHO
               0504!, CPEH K MEHEH ECKA 3.44D./
              ACCORDING TO  0504!, THE MEAN CYCLE OF LIGHT VA-
              RIATIONS IS 3.44D.
FK     AQL    D=0.02P. HA/DEPT OF MIN II 0.03M. P VAR.
FM     AQL    B-V:+1.12, +1.50.
FN     AQL    B-V:+1.10, +1.39. P VAR.
FZ     AQL    VB A (B 11.5M, 14", 162G).
GM     AQL    BOMOEH T UV  0504!/UV TYPE IS POSSIBLE
               0504!.
GU     AQL    D=0.02P.
GV     AQL    COACHO  2089!, BETC HOBOOOHO./NOVA-LI-
              KE STAR ACCORDING TO  2089!.
GY     AQL    MAEP/MASER OH, SIO.
HK     AQL    HE CKEH T ISB./TYPE ISB IS NOT EXCLUDED.
HL     AQL    P VAR? BEA 15M, OTMEEHHA HA KAPTAX  2274,
              6996!, OOEHE KOTOPO COOTBETCTBET KOOP-
              HATAM, AHHM P OTKPT, COACHO  2274!
              OCTOHHA/THE 15M STAR SHOWN IN THE CHARTS
               2274, 6996! WITH CO-ORDINATES COINCIDENT WITH
              THOSE GIVEN AT THE DISCOVERY IS CONSTANT ACCOR-
              DING TO  2274!.
IM     AQL    P VAR. O/BEFORE J.D.2432772 MAX=2428064.707+
              +0.4569602D*E.
IO     AQL    VB A (B=IP AQL, 30", 101G).
IP     AQL    CM./SEE IO AQL.
IS     AQL    TECH CTHK./CLOSE COMPANION.
KL     AQL    B-V:+0, 78, +1.19,  A/H!=0.6.
KO     AQL    D=0.018P. MIN II 8.40. P VAR. MIN=2427550.565+
              +2.863859D*E (J.D.2426250-33000)  2462!; MIN=
              =2433888.366+2.863954D*E (J.D.2433000-39000).
              TEKE EMEHT/CURRENT ELEMENTS-CM.TA.
              /SEE TABLE.
KP     AQL    MIN II 10.43; MIN II-MIN I=0.50P; DII=DI.
KV     AQL    B HTEPBAE/DURING J.D.2429130-31370-CM.
              TA./SEE TABLE. B HTEPBAE J.D.2428308-
              -28433 HE BHA. MAX 2436015 EMEHTAM TAK-
              E HE OBETBOPET./DURING J.D.2428308-
              -28433 THE STAR WAS FAINT. MAX 2436015 ALSO IS
              NOT SATISFIED BY THE ELEMENTS.
LU     AQL    B  3158! AH P=102D  PEOOEHO CECTBO-
              BAHE KOEAH CPEHE BEH C P=1080D 
              A=0.4M./IN  3158! P=102D IS GIVEN, AND THE EXIS-
              TENCE OF THE VARIATION OF MEAN MAGNITUDE WITH P=
              =1080D AND DM=0.4M WAS SUSPECTED.
MV     AQL    K CTHK, AH PEE MEHEH CM-
              MAPHOO ECKA./CLOSE COMPONENT, THE RANGE IS
              GIVEN FOR COMBINED LIGHT.
NN     AQL    P KECK VAR?/CYCLIC P VARIATIONS?
NV     AQL    CPEH ECK MEHETC C P-900D-1000D  DM
              -0.6M./VARIATIONS OF MEAN LIGHT WITH P-900D-
              -1000D AND DM-0.6M.
OO     AQL    MIN II 9.8. P VAR. MIN I=2426892.0582+
              +0.5067954D*E (1932-1934), MIN I=2433925.3762+
              +0.5067943D*E  8072!. OCE/SINCE J.D.2438000-
              -CM.TA./SEE TABLE. OPMA KPBO ECKA
              MEHETC./THE SHAPE OF THE LIGHT CURVE VARIES.
OX     AQL    VAR 2 HA KAPTE /IN THE CHART FOR OW AQL.
PP     AQL     A/H!=-0.0. HE CKEH T CWA./CWA TYPE
              IS NOT EXCLUDED. COACHO/ACCORDING TO  3161!
              P VAR. MAX=2415229.15+24.0147D*E (J.D.2415228-
              -21064), MAX=2426576.14+24.074D*E (J.D.2426576-
              -29489). OCE/AFTER J.D.2432040 MAX=
              =2433141.78+23.994D*E. TEKE EMEHT
              /CURRENT ELEMENTS MAX=2436836.04+23.973D*E.
PZ     AQL    P VAR? COACHO/ACCORDING TO  5387!, O/BEFORE
              J.D.2428075 P=8.7555D; P=8.7504D
              (J.D.2428075-34725); OCE/SINCE J.D.2434725
              P=8.7573D. CM. TAKE/SEE ALSO  2274!. EMEH-
              T B TAE OBETBOPTEHO PECTABT
              HAEH OCE J.D.2433150. OPMA KPBO
              ECKA, O-BMOM, MEHETC./ELEMENTS IN
              THE TABLE ARE SATISFACTORY AFTER J.D.2433150.
              THE SHAPE OF THE LIGHT CURVE APPARENTLY VARIES.
QS     AQL    MIN II 5.97. VB (A 6.5M; B 6.7M, 0.18", 137G).
              P VAR.
QV     AQL    AHA OXA ABHOO MAKCMMA./THE EPOCH
              OF MAIN MAX IS GIVEN.
QY     AQL    D=0.016P. P VAR?
V 336  AQL    B-V:+1.17, +1.55.
V 337  AQL    M   II 9.09. P VAR. OPMA KPBO ECKA ME-
              HETC./THE SHAPE OF THE LIGHT CURVE VARIES.
V 340  AQL    D=0.05P. P VAR.
V 341  AQL    P VAR. DS=4.
V 342  AQL    ADS 12259 B (A 7.5M; B 20", 14G); D=0.032P. P
              BEBAETC/INCREASES (CM. TAKE/SEE ALSO
               2265, 4493!). O/BEFORE J.D.2435600 MIN=
              =2428023.550+3.390842D*E. B MAX HAA-
              ETC MCC HALFA  8074!. OPMA KPBO EC-
              KA  D, O-BMOM, MEHTC. O-BMO-
              M, MEHAETC AMTA  8075!./HALFA EMIS-
              SION OBSERVED AT MAX LIGHT  8074!. THE SHAPE
              OF THE LIGHT CURVE AND DAPPARENTLY VARY. DM
              PROBABLY DECREASES  8075!.
V 343  AQL    MIN II 10.7.
V 346  AQL    MIN II 9.1. ADS 13438 A (B 11.3M, 2", 245G).
              PBEEHHE B TAE EMEHT ECTBT
              C J.D.2437000. OPMA MIN I MEHETC  7001!.
              /ELEMENTS IN THE TABLE ARE VALID AFTER
              J.D.2437000. THE SHAPE OF MIN I VARIES  7001!.
V 348  AQL    D=0.08P.
V 352  AQL    PO BOMOHO AHETAPHO TMAHHOCT/THE
              NUCLEUS OF THE SUPPOSED PLANETARY NEBULA P.K.
              37-3.3G.
V 356  AQL    VB A (B 0.2").
V 367  AQL    EMEHT OBETBOPT HAEHM TOKO
              B HTEPBAE J.D.2436450-37960. CXOHA C
              S VUL (SRD)./THE ELEMENTS ARE SATISFACTORY
              ONLY DURING J.D.2436450-37960. RESEMBLES
              S VUL (SRD).
V 368  AQL    VB A (B 0.17", 140G).
V 374  AQL    VB A (B-0.2', -270G).
V 406  AQL    MIN II 13.3:.
V 407  AQL    P VAR; EMEHT COEPAT HEHEH EH:
              /THERE IS NONLINEAR TERM IN THE ELEMENTS:
              +1.51D*10**-9*E**2.
V 409  AQL    MIN II 12.2. O POM CTOHK CEKTP
              A2-A3./SPECTRAL TYPE FROM ANOTHER PUBLICATION
              IS A2-A3.
V 411  AQL    AHA OXA MIN./EPOCH OF MIN IS GIVEN.
V 417  AQL    MIN II 11.5. P VAR. O/BEFORE J.D.2439000:
              MIN=2428427.127+0.3701251D*E.
V 421  AQ1    P VAR?
V 423  AQ1    EMEHT POH /ELEMENTS ARE VALID
              FOR J.D.2426900-28000. B HTEPBAE/DURING
              J.D.2429020-31670 BOH HATEHO H-
              HEE  OTCTCTBT/THE WAVES ARE MUCH LON-
              GER OR ABSENT.
V 433  AQ1    BOH 26D-80D C DM=0.1M-0.9M. CPEH
              ECK KOEETC C EMEHTAM MAX=
              =2438312+648D*E/WAVES OF 26D-80D DURATI-
              ON WITH DM=0.1M-0.9M. THE MEAN LIGHT VARIES
              ACCORDING TO THE FORMULA MAX=2438312+
              +648D*E.
V 461  AQ1    TECH CTHK-15.5M, AH PEE CM-
              MAPHOO ECKA./CLOSE COMPONENT-15.5M, THE
              RANGE OF COMBINED LIGHT IS GIVEN.
V 467  AQ1    BOH 40D-72D. CPEH ECK KOEETC C
              P-1400D./WAVES OF 40D-72D DURATION. THE
              MEAN LIGHT VARIES WITH P-1400D.
V 473  AQ1    HOA HAAETC P-330D./P-330D IS SO-
              METIMES OBSERVED.
V 476  AQ1    BOMOEH T EW C BOHM EPOOM. E-
              MEHT OEH HA KOPOTKOM HTEPBAE HA-
              EH./EW TYPE WITH DOUBLED PERIOD IS
              POSSIBLE. ELEMENTS ARE BASED ON A SHORT SERIES
              OF OBSERVATIONS.
V 483  AQ1    B OACT PACCEHHOO BEHOO CKOEH
              /IN THE FIELD OF THE OPEN CLUSTER NGC 6709.
V 486  AQ1    CM./SEE V 483 AQ1.
V 493  AQ1    B-V:+1.10, +1.38.
V 495  AQ1    D=0.06P:.
V 496  AQ1    B-V:+1.07, +1.28. EMEHT AH  OX
              OCE J.D.2428000./ELEMENTS ARE GIVEN FOR
              EPOCHS AFTER J.D.2428000.
V 497  AQ1    VB A (B 16.5M, 9", -0G).
V 524  AQ1    EPEMEHHA-NR OT BE, OTMEEHHO HA
              KAPTE B  2317!./THE VARIABLE IS NR FROM THE
              STAR SHOWN IN THE CHART IN  2317!.
V 527  AQ1    BOMOEH T IS./IS TYPE IS POSSIBLE.
V 528  AQ1    VB A (B 16.5M, 11", 59G).
V 535  AQ1    VB. PAEETC HA AOMAPCKOM ATACE;
              BOCTOH KOMOHEHT-KPACH. COACHO
               1943!, CTPA./TWO COMPONENTS ARE SEEN
              ON PALOMAR PRINTS, EASTERN OF THEM BEING RED.
              ACCORDING TO  1943!, RAPID VARIABLE.
V 537  AQ1    BOMOEH P=200D./POSSIBLE P=200D.
V 538  AQ1    BOMOEH P=375D./POSSIBLE P=375D.
V 558  AQ1    BOMOEH P=187D./POSSIBLE P=187D.
V 571  AQ1    BOMOEH P=185.5D./POSSIBLE P=185.5D.
V 572  AQ1    B-V:+0.65, +0.87. P VAR. O/BEFORE
              J.D.2435500 P-3.7686D. CM. TAKE/SEE ALSO
               8637!.
V 586  AQ1    BPEMEHAM HEPABHOCT, HO EPOHOCT,
              O-BMOM, BOCCTAHABBAETC./IRREGULARI-
              TIES ARE SOMETIMES OBSERVED, BUT THEN THE PE-
              RIODICITY IS PROBABLY RESUMED.
V 596  AQ1    HAOMHAET/RESEMBLES S VUL.
V 599  AQ1    MIN II 6.73. COACHO  8083!, BOMOHO, OCTO-
              HHA./ACCORDING TO  8083!, MAY BE CONSTANT.
V 600  AQ1    B-V:+1.36, +1.70. BOMOHO, O J.D.2428000
              EPO  PM  8632!./BEFORE J.D.2428000
              ANOTHER VALUE OF P IS POSSIBLE  8632!.
V 602  AQ1    D=0.02P. MIN II 12.7.
V 603  AQ1    SB (P=0.13854D  3169!). ECK BHE BCK
              CTBAET KOEAH ATMEHHOO TA C
              DM=0.30M, MIN I=2444401.399+0.1377D*E (D-
              -0.2P). OPMA KPBO ECKA  HA MH-
              MMOB MEHTC OT KA K K. B MH-
              MMAX ECK KTPET, TO, BMO, CB-
              AHO C CECTBOBAHEM OPEO THA
               4500!/OUTSIDE THE OUTBURST THERE ARE VARIA-
              TIONS OF LIGHT (ECLIPSES) WITH DM=0.30M,
              MIN I=2444401.399+0.1377D*E (D-0.2P). THE
              SHAPE OF THE LIGHT CURVE AND THE DEPTH OF MI-
              NIMA DIFFER FROM CYCLE TO CYCLE. THE BRIGHT-
              NESS IN MINIMA SHOWS FLUCTUATIONS APPARENT-
              LY CONNECTED WITH THE PRESENCE OF A HOT SPOT
               4500!.
V 605  AQ1    HKAHA EPEMEHHA. B 8" NR OT BE
              17M. MIN-20M PG. OTO OKPECTHOCTE
               6041, 6042!. O B KPBO ECKA HAOM-
              HAET SN B NGC 1058  ETA CAR  6040!. PO-
              OTEH MAX C KTAM HA-
              AC  B 1918-1924. B 1921 CEKTP 
              KACCPOBAH KAK R  2464!. BEA HA-
              XOTC BHTP CTAPO AHETAPHO TMAH-
              HOCT A 58  MOET T EE POM./A UNIGUE
              VARIABLE. 8" NR FROM A 17M STAR. MIN-20M PG.
              PHOTOGRAPHS OF THE FIELD  6041, 6042!. THE
              LIGHT CURVE RESEMBLES THOSE OF THE SN IN NGC
              1058 OR OF ETA CAR  6040!. THE ONLY MAX OBSER-
              VED, WITH FLUCTUATIONS, OCCURED IN 1918-1924.
              IN 1921 THE SPECTRAL TYPE WAS FOUND TO BE R
               2464!. THE STAR IS INSIDE THE OLD PLANETARY NE-
              BULA A 58 AND MAY BE ITS NUCLEUS.
V 609  AQ1    MIN II 11.9.
V 615  AQ1    P VAR? MAX=2428046+364D. E (J.D.2428038-
              -31343)  1091!.
V 616  AQ1    D=0.04P. EMEHT TPET POBEPK./ELE-
              MENTS REGUIRE VERIFICATION.
V 618  AQ1    HE CKEH BBOE MEH EPO./TWICE
              SHORTER PERIOD IS NOT EXCLUDED.
V 637  AQ1    CM./SEE V 618 AQ1.
V 638  AQ1    CM./SEE V 618 AQ1.
V 640  AQ1    MIN II 12.8.
V 647  AQ1    HEOO/SLIGHT MIN II  1091!.
V 663  AQ1    BOMOEH P=194.5D/P=194.5D IS POSSIBLE.
V 666  AQ1    KAAH CMMAPH ECK C PEECTBE
              BEO 16.5M. OTEHO B MIN OEHEHA
              -17M PG./THE RANGE IS GIVEN FOR COMBINED MA-
              GNITUDE WITH A PRECEDING 16.5M STAR. SEPARATELY
              WAS FOUND-17M PG NEAR MIN.
V 672  AQ1    P VAR? BOMOEH EKT AKO/BLAZHKO EF-
              FECT IS POSSIBLE  3113!.
V 678  AQ1    P VAR. O/BEFORE J.D.2429723 MAX=2429723+
              +120.6D*E.
V 688  AQ1    MIN II 10.8. DII=0.15P.
V 694  AQ1    D=0.13P. VB (1"), CTHK HA -1M CAEE E-
              PEMEHHO  1881!, BOMOHO, CKAAET PBO-
              ME AHHE/A COMPANION-1M FAINTER THAN
              THE VARIABLE  1881! MAY HAVE AFFECTED THE DATA
              GIVEN.
V 699  AQ1    MIN II 13.75.
V 706  AQ1    DS=0:.
V 708  AQ1    BOH C P-65D HAKABATC HA MEEHHOE
              KOEAHE CPEHEO ECKA C P-1350D
              (J.D.2437124-40512)  6025!. COACHO  0773!,
              BOH C P-100D-150D (J.D.2427543-31318).
              /P-65D WAVES SUPERIMPOSED ON SLOW VARIATION
              OF MEAN BRIGHTNESS WITH P-1350D (J.D.2437124-
              -40512)  6025!. ACCORDING TO  0773! WAVES
              WITH P-100D-150D (J.D.2427543-31318).
V 714  AQ1    D=0.05P.
V 724  AQ1    MIN II 11.57.
V 733  AQ1    P VAR? O/BEFORE J.D.2434500, BOMOHO,
              /POSSIBLY MAX=2434453.72+6.17687D*E  0001!.
V 734  AQ1    VB A? (B 16.1M?).
V 743  AQ1    EA./WHITE. SRD?
V 755  AQ1    BOMOH HECKOKO MEHEHHE EMEHT/
              ALTERNATIVE ELEMENTS: MIN=2429195.290+
              +1.01598D*E.
V 765  AQ1    B-V:+0.70, +0.80.
V 766  AQ1    HE CKEH T EW./EW TYPE IS NOT EXCLUDED.
V 769  AQ1    D=0.05P?
V 770  AQ1    MIN II 14.0.
V 771  AQ1    COACHO/ACCORDING TO  3165! UG.
V 774  AQ1    BOMOHO, CXOHA C UV BOO./POSSIBLY RESEM-
              BLES UV BOO.
V 777  AQ1    BOMOEH P=111.5D./P=111.5D IS POSSIBLE.
V 784  AQ1    MIN II 14.8.
V 794  AQ1    CTPE KOEAH C DM O 1.5M HAKABA-
              TC HA MEEHHE. BOMOHO, OTHOCTC K
              "OPAM" TA XPRM. CEKTP EKPH C
              PAMTM MCCM  OM KOHTH-
              MOM  8676!./RAPID CHANGES WITH DM UP TO
              1.5M SUPERIMPOSED ON SLOW ONES. MAY BELONG TO
              "POLARS" OF XPRM TYPE. PECULIAR SPECTRUM
              WITH BROAD EMISSIONS AND BLUE CONTINUUM  8676!.
V 800  AQ1    VB. COACHO/ACCORDING TO  6072! UGZ.
V 801  AQ1    VB A (B 15.1M SP).
V 803  AQ1    MIN II 14.8.
V 804  AQ1    MIN II 12.8. B/IN MAX B-V=+0.61.
V 805  AQ1    MIN II 7.90, DII=0.11P.
V 808  AQ1    MIN II 13.3.
V 812  AQ1    VB A (B 16M SP, C 16M SF).
V 814  AQ1    VB A (B 16.5M SP).
V 822  AQ1    MIN II 7.07. ADS 12538 A (B 10.1M, 1", 67G).
              OPMA KPBO ECKA MEHETC. BOMOHA
              ACCMETP KPBO ECKA. B MIN I OKAATE
              BETA (U-B) KPACHEE, B MIN II-OEE CPE-
              HEO./THE SHAPE OF THE LIGHT CURVE VARIES.
              (U-B) INDEX IN MIN I IS REDDER AND MIN II IS
              BLUER THAN AVERAGE.
V 829  AQ1    EPO, MOET T, CEET BOT./TWICE
              LONGER P IS POSSIBLE.
V 836  AQ1    BOMOEH T RR ( 0085!, O EM CBETECTB-
              ET TAKE CEKTP  8676!)./RR TYPE IS POSSIBLE
              ( 0085!; IT IS SUGGESTED ALSO BY THE SPECTRUM
               8676!).
V 850  AQ1    B EHTPE AHETAPHO TMAHHOCT/IN THE CENT-
              RE OF THE PLANETARY NEBULA P.K. 37-6.2.
V 866  AQ1    MIN II 14.8. COACHO  6026!, HA MIN II
              0.4M, T EB./ACCORDING TO  6026!, THE DEPTH
              OF MIN II 0.4M, EB TYPE.
V 867  AQ1    P VAR?
V 871  AQ1    MIN II 14.5, MIN II-MIN I=0.425P. BOMOH
              ECKE MEHEH ECKA B PEEAX
              13.3-13.6. ATMEH POCXOT OT POBH 13.6
              /PHYSICAL CHANGES IN THE RANGE 13.3-13.6 ARE
              POSSIBLE. ECLIPSES START FROM THE 13.6M LEVEL.
V 872  AQ1    MIN II 15.7:. BOMOHO BEHE H AC
              /APSIDAL MOTION IS POSSIBLE.
V 873  AQ1    P VAR? CPEH ECK MEHETC B PEEAX
              13.8-14.0./THE MEAN LIGHT VARIES IN THE RANGE
              13.8-14.0.
V 875  AQ1    EA. COACHO  6004! CTPA. BOMOHO,
              UGZ  IA./WHITE. ACCORDING TO  6004!, RA-
              RID. POSSIBLY UGZ OR IA.
V 877  AQ1    VB A (B 16.5M NF).
V 882  AQ1    BOMOEH EKT AKO./BLAZHKO EFFECT IS
              POSSIBLE.
V 885  AQ1    MIN II 14.9:. BOMOH BEHE H AC
               MEHEH OPM KPBO ECKA./APSIDAL
              MOTION AND CHANGES OF THE SHAPE OF THE LIGHT
              CURVE ARE POSSIBLE.
V 888  AQ1    BOMOH EH PACCEHHOO CKOEH
              NGC 6738./A POSSIBLE MEMBER OF THE OPEN CLUS-
              TER NGC 6738.
V 889  AQ1    MIN II 9.0. MIN II-MIN I=0.35P. BOMOHO B-
              EHE H AC./APSIDAL MOTION IS POSSIB-
              LE.
V 890  AQ1    NOVA AQ1 1946=ACTEPO/ASTEROID N258 TYCHE
               9038!.
V 891  AQ1    MIN II 15.8.
V 895  AQ1    P VAR. MAX=2430931.435+0.265108D*E
              (J.D.2426920-35010)  2267!. B HTEPBAE
              /DURING J.D.2441890-42290-CM. TA./SEE
              TABLE.
V 907  AQ1    MIN II 15.7.
V 912  AQ1    OPMA KPBO ECKA MEHETC./THE SHAPE OF
              THE LIGHT CURVE VARIES.
V 914  AQ1    B  8717! OOHO HAEATOHO/P=3.336217D
              IS GIVEN IN  8717! BY MISPRINT.
V 919  AQ1    MIN II 13.8.
V 920  AQ1     OEE PAHHX HAEH/F OR EARLIER OB-
              SERVATIONS MAX=2429458.400+0.4955033D*E.
V 922  AQ1    EMEHT HE BOHE HAEH./ELEMENTS ARE
              NOT QUITE RELIABLE.
V 923  AQ1    HEOHA BEA C OOOKO  1884!. CXO-
              HA C EW LAC. H HE PACPEH BPAEH-
              EM, H NA I KE. MEHEH ECKA E-
              POH: MIN=2436458.66+0.8518D*E. P-
              HA MEHEH, BOMOHO, CBAHA C BPAE-
              HEM BE  HEOHOPOHM PACPEEEH-
              EM PKOCT O EE CK  3178!. PO -
              H B CEKTPE MEHTC. PACPEHE OOO-
              K PEKPATOC B 1965, TO, BMO, PBE-
              O K PABT B HE HEOHOPOHOCTE  PAC-
              PEH POE H BOOPOA  4525!.
              /UNUSUAL SHELL STAR  1884!. SIMILAR TO EW LAC.
              HE LINES ARE WIDENED BY THE ROTATION, NAI LINES
              ARE NARROW. LIGHT CHANGES ARE PERIODIC: MIN=
              =2436458.66+0.8518D*E. THE CAUSE OF VARIA-
              TIONS IS PROBABLY CONNECTED WITH THE ROTATION
              AND THE INHOMOGENEOUS BRIGHTNESS DISTRIBUTION
              OVER THE DISK OF THE STAR  3178!. PROFILES OF
              SPECTRAL LINES VARY. THE EXPANSION OF THE ENVE-
              LOPE TERMINATED IN 1965, WHICH APPARENTLY LED
              TO THE DEVELOPMENT OF INHOMOGENEITIES AND TO
              THE BROADENING OF HYDROGEN LINE PROFILES  4525!.
V 925  AQ1    HEKOTOPE HAATE OTMEAT OCTOHCT-
              BO ECKA  3165!./SOME OBSERVERS FOUND CONS-
              TANT BRIGHTNESS  3165!.
V 929  AQ1    KOPOTK EPO./SHORT PERIOD.
V 936  AQ1    CM./SEE V 929 AQ1.
V 947  AQ1    COACHO  5412!, HE CKEH CTPE HE-
              PABHE MEHEH. COACHO  0504! O-
              CTOHHA./ACCORDING TO  5412!, RAPID IRREGULAR
              CHANGES ARE NOT EXCLUDED. ACCORDING TO  0504!,
              CONSTANT.
V 955  AQL    MIN II 14.9,  II=0.13P.
V 956  AQL    MIN II 14.2. EMEHT TPET OTBEPE-
              H./ELEMENTS NEED CONFIRMATION.
V 957  AQL    P VAR. MAX=2428154.960+0.6051327D*E
              (J.D. 2421871-28105).
V 958  AQL    VB A (B 17.0M, 0.2' P; C-CEKA OEE PKA/
              SLIGHTLY BRIGHTER, 0.1'F). OEHBAC CMMAP-
              H ECK A  C./COMBINED MAGNITUDE OF A
              AND C IS GIVEN.
V 964  AQL    MIN II 13.7.
V 969  AQL    BOMOEH EKT AKO./BLAZHKO EFFECT IS
              POSSIBLE.
V 981  AQL    MIN II 14.5.
V 991  AQL    BOMOEH T IS./IS TYPE IS POSSIBLE.
V 992  AQL    B  4260! AH P=110D./ACCORDING TO  4260!,
              P=110D.
V 998  AQL    OOEHE COBAAET C AHETAPHO TMAH-
              HOCT/THE POSITION COINCIDES WITH THE PLA-
              NETARY NEBULA P.K.50-3.1G.
V 999  AQL    HAEH ECEBA  7806! HE OBETBO-
              PT TAHM EMEHTAM./TSESSEVICH'S
              OBSERVATIONS  7806! DO NOT AGREE WITH THE ELE-
              MENTS IN THE TABLE.
V 1017 AQL    EMEHT HATC B POBEPKE./ELEMENTS
              NEED CONFIRMATION.
V 1033 AQL    P VAR?
V 1045 AQL    MIN II 13.5.
V 1046 AQL    P VAR?  8321!.MIN=2427713.314+5.28303D*E
               4027!. BOMOEH HEOO EKT OTPA-
              EH./SLIGHT REFLECTION EFFECT IS POSSIBLE.
V 1064 AQL    K/CYCLES 295D-410D.
V 1072 AQL    SP KOMOHEHT TECHO AP/SP COMPONENT
              OF A CLOSE PAIR.
V 1075 AQL    D=0.04P. MIN II 13.6.
V 1076 AQL    VB A (B 18M TECH, PEECTBET/CLOSE
              PRECEDING).
V 1086 AQL    VB. EPEMEHEH, BEPOTHO, SF KOMOHEHT.
              /PROBABLY THE VARIABLE IS THE SF COMPONENT.
V 1093 AQL    BOMOEH T IA./IA TYPE IS POSSIBLE.
V 1095 AQL    P VAR. OCE/AFTER J.D.2429048-CM.TA.
              /SEE TABLE, PAHEE/EARLIER MAX=2427322+
              +42.68D*E. AMETHO HE OKPAEHA./NOT COLO-
              URED APPRECIABLY.
V 1096 AQL    MIN II 13.3.
V 1097 AQL    MIN II 14.0.
V 1101 AQL    BOMOEH T UGZ  3156!. /POSSIBLY UGZ
              TYPE  3156!.
V 1113 AQL    EPO, BOMOHO, BBOE MEHE. /THE PE-
              RIOD MAY BE TWICE SHORTER.
V 1117 AQL    MIN II 16.6.
V 1125 AQL    MIN II 16.0.
V 1140 AQL    P VAR?
V 1154 AQL    MIN II 14.8; MIN II-MIN I=0.70P.
V 1165 AQL    COACHO  4564! OCTOHHA. B PAOTE  3932!
              HE PAEEHA C KO BEO, C EM CB-
              AHO, O-BMOM, CKAEHE KPBO EC-
              KA. /ACCORDING TO  4564!, CONSTANT. IN  3932!
              WAS NOT SEPARATED FROM A CLOSE COMPONENT
              WHICH PROBABLY LED TO DISTORTIONS OF THE LIGHT
              CURVE.
V 1166 AQL    BOMOEH T UG. /UG TYPE IS POSSIBLE.
V 1173 AQL    NF KOMOHEHT TECHO AP/NF COMPONENT OF
              A CLOSE PAIR.
V 1182 AQL    MIN II 8.65.
V 1184 AQL    MIN II 13.4.
V 1200 AQL    VB. EPEMEHHA-BOCTOH KPACH KOM-
              OHEHT. /THE VARIABLE IS THE EASTERN RED COM-
              PONENT.
V 12O4 AQL    VB. EPEMEHEH BOCTOH KOMOHEHT. /THE
              VARIABLE IS THE EASTERN COMPONENT.
V 12O8 AQL    BEA 9.06M B 1' K  MEET OEE MU C
              EPEMEHHO. /A COMMON PRORER MOTION STAR
              9.06M IN 1' TO THE SOUTH.
V 1248 AQL    BOMOEH T UG. /UG TYPE IS POSSIBLE.
V 1251 AQL    KPACHA. /RED.
V 1261 AQL    B HD CEKTP K2. /SPECTRAL TYPE K2 IN HD.
V 1269 AQL    VB. EPEMEHEH AAH KOMOHEHT. /THE
              VARIABLE IS THE PRECEDING COMPONENT.
V 1281 AQL    KPACHOBATA. BOMOEH T SRD. /REDDISH.
              SRD TYPE IS POSSIBLE.
V 1286 AQL    EPO, BOMOHO, CAH. /POSSIBLY THE
              PERIOD IS ACCIDENTAL.
V 1288 AQL    ADS 12182 A (B 12.3M, 36", 287G).
V 1291 AQL    EMEHT OPEEEH O MEHEHM MA-
              HTHOO O. PBEEHA OXA MIN HAP-
              EHHOCT MAHTHOO O. /THE ELEMENTS
              HAVE BEEN DETERMINED ON THE BASE OF MAGNE-
              TIC FIELD VARIATIONS. THE EPOCH OF MINIMUM
              INTENSITY OF THE MAGNETIC FIELD IS GIVEN.
V 1295 AQL    BEA C OOOKO. HAAC PEKE
              MEHEH  B CEKTPE  5240!. EPEMEHHOCT
              BP  EPOECKA, XOT BOMOEH
              P-100D. HOA HAATC KTA
              ECKA A  HECKOKO HE  5880!. K -
              TOK  6277!. OPOHOE CEKTPAHOE CCE-
              OBAHE, C KAAHM HA CTEEHE BEE-
              CTBA C OBEPXHOCT, CM.  4739!. AMETHOE
              MAHTHOE OE  4435!. /SHELL STAR. DRAMA-
              TIC SPECTRAL CHANGES WERE OBSERVED  5240!.
              THE VARIABILITY IS HARDLY PERIODIC, THOUGH
              P-100D IS POSSIBLE. SOMETIMES LIGHT FLUCTUA-
              TIONS ON SEVERAL DAYS'TIME SCALE ARE OBSER-
              VED  5880!. IR EXCESS  6277!. FOR A DETALILED
              SPECTROSCORIC STUDY, WITH EVIDENCE FOR THE
              OUTFLOW OF MATTER FROM THE SURFACE, SEE  4739!.
              CONSIDERABLE MAGNETIC FIELD  4435!.
V 1297 AQL    D=0.05P? MIN II 14.5.
V 1298 AQL    MU ALFA=-0.0392S,  MU DELTA=-1".330. CTHK BE. /
              THE COMPANION OF THE STAR BD+4G4048 (RO=
              =73".8, TETA=151G5). OHA  CAEX O
              CBETMOCT  BECTHX BE (MV=+19M).
              /ONE OF THE ABSOLUTELY FAINTEST KNOWN STARS
              (MV=+19M).
V 1300 AQL    I_K:+5.2, +6.5. HOA MAEPHA MCC/
              SOMETIMES MASER EMISSION CO, SIO, OH.
V 1302 AQL    HKAH K O'EKT /A UNIQUE IR OBJECT
              IRC+10420. B_V=+2.7, U_B=+1.9. OH-,
              H2O-, SIO-MAEP/MASER. COACHO  7437!,
              O PACPEEEH HEP B K OACT
              CEKTPA (1-22MU) CXOHA C TETA CAR. B CEKTPE
              HAATC MCC HETPAHX ATOMOB
              METAOB. BOPACTA B ECKE C 1925 O
              1970;MAX-1970. /ACCORDING TO  7437!, THE
              ENERGY DISTRIBUTION IN THE IR SPECTRUM (1-22MU)
              RESEMBLES THAT OF ETACAR. EMISSIONS OF NEUT-
              RAL METALS ARE OBSERVED IN THE SPECTRUM. INCRE-
              ASED IN BRIGHTNESS DURING 1925-1970;MAX-1970.
V 1323 AQL    TECHA/CLOSE VB;VAR-CEBEPH KOMO-
              HEHT/NORTHERN COMPONENT.
V 1331 AQL    MIN II 7.95. COACHO/ACCORDING TO  4619!
              P=1.364076D.
V 1333 AQL    AQL X-1. BOMOH MEHEH ECKA C
              P-1.28D-1.31D, CBAHHE C OPTAHM
              BEHEM  4625!. HAATC BCK,
              XAPAKTEPHE  TA XB  4757!. BHE HO-
              BOOOHX BCEK LX/LOPT=500, BO BPE-
              M BCEK LX/LOPT=5000./LIGHT VARIATI-
              ONS WITH P-1.28D-1.31D DUE TO ORBITAL MOTI-
              ON ARE POSSIBLE  4625!. BURSTS CHARACTERIS-
              TIC OF THE XB TYPE ARE OBSERVED  4757!. LX/
              LOPT=500 OUTSIDE NOVA-LIKE BURSTS, LX/LOPT
              =5000 DURING BURSTS.
V 1336 AQL    B/IN 1.6' W OT/FROM MXB 1916-05. BOMO-
              EH T M./M TYPE IS POSSIBLE.
V 1340 AQL    D=0.06P? BOMOH ECKE MEHEH
              ECKA B MAX. /INTRINSIC LIGHT VARIATIONS IN
              MAX ARE POSSIBLE.
V 1341 AQL    MIN II 13.4. P=0.3586768D BOMOEH /IS PO-
              SSIBLE.
V 1343 AQL    SS 433. <B-V>=+2.0. ACCOPOBAHA C SNR
              W 50. CPEH ECK MEHETC B PEEAX
              14.0-14.6 V C EMEHTAM: MAX= 2443662.5+
              +165.5D*E.  0512!. HA MIN I MEHETC
              OT 0.2M O 0.9M V, HA MIN II - OT 0 O
              0.4M V. B CEKTPE - BE CCTEM MCCOH-
              HX H H, HEI, HEII: "CTAOHAPHA", CO-
              OTBETCTBA MEHEH VR OT 300 O
              150 KM/C C P=13.1D,  "PETBCTCKA", CO-
              OTBETCTBA MEHEHM VR OT +50000
              O -35000 KM/C C P=165.5D. CCEOBAHE
              CEKTPA  0535!. CCTEMA, O-BMOM, CO-
              CTOT  O-B BE, AOHE CBO
              BHTPEHH OOCT POA,  KOMAKTHOO
              O'EKTA, OKPEHHOO AKKPEOHHM CKOM,
              PEECCPM C P=165.5D.  CCTEM BTE-
              KAT C PETBCTCKO CKOPOCT (0.27C) B POT-
              BOOOHX HAPABEHX BE CTP, COCTOE
               OTHX CCTKOB BEECTBA. CBETMOCT C-
              KA COCTABET HE MEHEE 60% OE CBETMOCT
              CCTEM  0926, 0953!. BOMOHO, BA CBEPX-
              HOBA, BCXHBA HE OEE 10**4 ET HAA.
              /ASSOCIATED WITH THE SNR W 50. MEAN LIGHT VA-
              RIES IN THE RANGE 14.0-14.6 V ACCORDING TO THE
              ELEMENTS MAX=2443662.5+165.5D*E  0512!.
              THE DEPTH OF MIN I VARIES FROM 0.2M TO 0.9M V,
              THE DEPTH OF MIN II VARIES FROM 0 TO 0.4M V. TWO
              SYSTEMS OF H, HEI, HEII EMISSION LINES ARE OB-
              SERVED IN THE SPECTRUM: THE "STATIONARY" SYS-
              TEM CORRESPONDING TO VR CHANGES FROM 300 TO
              150 KM/S WITH P=13.1D, AND THE "RELATIVISTIC"
              ONE, CORRESPONDING TO VR CHANGES FROM +50000
              TO-35000 KM/S WITH P=165.5D. THE SPECTRAL
              STUDY  0535!. THE SYSTEM APPARENTLY CONSISTS
              OF AN O-B STAR FILLING ITS INNER ROCHE LOBE
              AND A COMPACT OBJECT SURROUNDED BY AN ACCRE-
              TION DISC WICH IS PRECESSING WITH P=165.5D.
              TWO JETS CONSISTING OF DENSE CONDENSATIONS OF
              MATTER EMERGE FROM THE SYSTEM WITH RELATIVISTIC
              VELOCITY (0.27 C) IN OPPOSITE DIRECTIONS. THE
              LUMINOSITY OF THE DISC AMOUNTS TO NOT LESS
              THAN 60% OF THE TOTAL LUMINOSITY OF THE SYSTEM
               0926, 0953!. THE OBJECT MAY BE A FORMER SU-
              PERNOVA WHICH BURSTED NOT MORE THAN 10**4
              YEARS AGO.
V 1345 AQL    MIN II 14.3:, MIN II-MIN I=0.46P.
V 1349 AQL    MAX-17 PG.
V 1352 AQL    VB A (B 14.5M, 6", 175G).
V 1353 AQL    MIN II 10.9.
V 1355 AQL    MIN II 13.3.
V 1357 AQL    BOMOHO/POSSIBLY P=1.051D.
ETA    AQL    P VAR. P=7.176344D (J.D. 2373000-95100),
              P=7.176455D (J.D. 2395100-2412100). OCE
              /SINCE J.D. 2412100-CM. TA./SEE TABLE.
               BCEO HTEPBAA HAEH/FOR THE
              WHOLE INTERVAL MAX=2442794.773+7.176735D*E+
              +2.18D*10**-8*E**2  8632!. B  AAOHE A-
              METHO EHE BEPOTHOO CTHKA -
              BE AOV./IN THE UV BAND THE LIGHT OF A
              POSSIBLE AOV COMPARION IS APPARENT.
SIGMA  AQL    ADS 12737 A (B 12.34M, 48", 328G). HA/
              DEPTH OF MIN II 0.1M. B  4627! AHO P=
              =1.950271D O CEKTPAHM AHHM./IN
               4627! P=1.950271D IS GIVEN ACCORDING TO
              SPECTROSCORIC DATA.
R      ARA    MIN II 6.2. VB A (B 8.2MV,  4", 123G).
S      ARA    (K-B)2=0.09. P VAR  1932, 3126!. MAX=2416284.792+
              +0.45188910D*E (J.D. 2414000-19000);MAX=
              =2419149.797+0.45188581D*E (J.D. 2419000-
              -30000)  0752!. OCE/SINCE J.D. 2441000 - CM.
              TA./SEE TABLE. HA BCEM HTEPBAE C OCTATO-
              HO TOHOCT/FOR THE WHOLE INTERVAL, WITH SUF-
              FICIENT ACCURACY, MAX=2420047.2382+
              +0.451888176D*E-1.36D*10**-10*E**2  3126!.
T      ARA    VB A (B 11.0M, 34", 60G).
X      ARA    OTMEEHA HA KAPTE  S 5809./SHOWN IN THE
              CHART FOR S 5809.
RT     ARA    COACHO KHHOH  1944!, OTKPBE EPEMEH-
              HOCT ECKA TO BE, OHA MEET CTHKA
              12.0M, PACOOEHHOO HA 0.1M K W  HECKOKO
              CEBEPHEE EPEMEHHO. KHHOH OTMEAET, TO B
              MIN EPEMEHHA CTAHOBTC CAEE CTHKA.
              XOMECTEP  0016!  H-AOKHA  0624!
              HE OHAP HKAKX PHAKOB CECTBOBA-
              H CTHKA. COACHO  0624!, CPEH K
              -78D,  BOMOEH T RVA./ACCORDING TO
              CANNON  1944! WHO DISCOVERED THE STAR'S VARIABI-
              LITY, A COMPANION 12.0M IS PRESENT IN 0.1M TO W
              AND SOMEYHAT TO THE NORTH FROM THE VARIABLE. CAN-
              NON POINTS OUT THAT AT MIN LIGHT THE VARIABLE BECO-
              MES FAINTER THAN THE COMPANION. NO SIGN OF THE
              COMPANION'S EXISTENCE WAS FOUND BY HOFFMEISTER
               0016! AND BY PAYNE-GAPOSCHKIN  0624!. ACCOR-
              DING TO  0624!, THE MEAN CYCLE IS-78D, AND RVA
              TYPE IS POSSITLE.
RW     ARA    D=0.022P. MIN II 8.91. BOMOH MEHEH OP-
              M KPBO ECKA, CBAHHE C AOBM OTO-
              KAM  OPM THOM./CHANGES OF THE SHAPE
              OF THE LIGHT CURVE DUE TO GASEOUS STREAMS OR A HOT
              SPOT ARE POSSIBLE.
TT     ARA    BOMOHO PCTCTBE B CEKTPE OOC ZRO
               3181!./ZRO BANDS MAY BE PRESENT IN THE SPECTRUM
               3181!.
TV     ARA    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              NGC 6208.
TX     ARA    VB A (B 16.5M). BOMOEH OOBHH EPO./
              TWICE SHORTER PERIOD IS POSSIBLE.
XX     ARA    MIN II 14.1.
YY     ARA    HE CKEHO, TO EPEMEHHA BETC ATMEH-
              HO  HEPABHO  0424!./THE STAR'S BEING
              AN ECLIPSING OR IRREGULAR VARIABLE  IS NOT EXCLUDED
               0424!.
AA     ARA    MIN II 13.3.
AD     ARA     A/H!=-0.4.
AE     ARA    VB A (B 12M, 0.3' SF). P.K. 344-8.1. KOMAKTHA
              AHETAPHA TMAHHOCT  CMOTECKA
              BEA. HAATC HEPABHE BHEAHE
              BEEH ECKA HA 3M-4M C HTEPBAAM B
              HECKOKO ET  0255!. OCEHE CEKTPA-
              HX AHHX  8076!./A COMPAST PLANETARY NEBULA
              OR A SYMBIOTIC STAR. IRREGULAR ABRUPT BRIGHTENINGS
              BY 3M-4M SEPARATED BY SEVERAL YEARS ARE OBSER-
              VED  0255!. THE SPECTRAL DATA ARE DISCUSSED IN
               8076!.
AF     ARA    MIN II 13.8.
AW     ARA    O/BEFORE J.D. 2417300 MAX=2412600+186D*E.
BQ     ARA    BOHE MAKCMM C HTEPBAOM 10D-20D
              ME HM  MIN II 12.8./DOUBLE MAXIMA SEPA-
              RATED BY 10D-20D, WITH MIN II 12.8.
CC     ARA    VB;EPEMEHHA - NF KOMOHEHT./THE VARIABLE IS
              NF COMPONENT.
CH     ARA    BEA OTMEEHA HA KAPTE OKPECTHOCTE 
              S 6062=V 466 ARA./NOTED ON THE FINDING CHART FOR
              S 6062=V 466 ARA.
CT     ARA    O/BEFORE J.D. 2420400 MAX=2413080+215D:*E;
              OCE/SINCE J.D. 2425000 - CM. TA./SEE TABLE.
DU     ARA    B-V:+0.52, +0.84. P VAR. MAX=2418145.560+
              +1.63999D*E (J.D. 2411000-21000);OCE/SINCE
              J.D. 2425000 - CM. TA./SEE TABLE.
EK     ARA    VB A (B 15M).
EL     ARA    O/BEFORE J.D. 2420400 MAX=2415140+332D*E;
              OCE/SINCE J.D. 2425000 - CM.  TA./SEE TABLE.
ER     ARA    MIN II 14.2.
EV     ARA    O/BEFORE J.D. 2420400 MAX=2413750+237D*E;
              OCE/SINCE J.D. 2425000 - CM. TA./SEE TABLE.
EZ     ARA    P VAR.
FU     ARA    HA MIN I 0.97M  0.89M, HA MIN II 0.20M
               0.23M COOTBETCTBEHHO B OX  ETX -
              AX./THE DEPTH OF MIN I IS 0.97M AND 0.89M,
              THE DEPTH OF MIN II IS 0.20M AND 0.23M IN BLUE AND
              YELLOW LIGHT, RESPECTIVELY.
GK     ARA    O/BEFORE J.D. 2417800 MAX=2414050+237D*E,
              OCE/SINCE J.D. 2418400 - CM. TA./SEE TABLE.
GM     ARA    MIN II 12.8.
HX     ARA    B-V:+0.23, +0.36. OP HA BOCXOE BETB/A
              HUMP ON THE ASCENDING BRANCH (FI=0.93P)  8118!.
KY     ARA    HAAC TOKO OH OCTP MAX J.D. 2428715-
              -712. BEA MOET T HOBO./ONLY ONE SHARP
              MAX (J.D. 2428715-712) WAS OBSERVED. POSSIBLY
              A NOVA.
KZ     ARA    VB A (B 14.1M SP).
LP     ARA    D=0.04P? MIN II 10.5?
LQ     ARA    B 1959 . BPEMEHAM CTPO MEHAC HA 0.5M
              OKOO 11M; OKPEHA TMAHHOCT  4001!./IN
              1959 RAPID VARIATIONS AT TIMES FOR 0.5M NEAR 11M
              WERE OBSERVED;SURROUNDED BY A NEBULA  4001!.
LR     ARA    MIN II 10.6.
LU     ARA    MIN II 10.1?
MQ     ARA    VB. EPEMEHHA - NF BEA./NF COMPONENT IS
              VARIABLE.
MR     ARA    B-V:+0.72, +0.8.  A/H!=-1.0. P VAR?
QR     ARA    OTMEEHA HA KAPTE  BV 1443./SHOWN IN THE
              CHARP FOR BV 1443.
QU     ARA    VB.
QW     ARA    EPEMEHHA - NP KOMOHEHT AP./THE VARIAB-
              LE IS NP COMPONENT OF THE PAIR.
QX     ARA    OTMEEHA HA KAPTE  S 5818./SHOWN IN THE
              CHARP FOR S 5818.
V 340  ARA    B-V:+1.25, +1.68.  A/H!=0.6.
V 341  ARA    BEA OA;A 4D P MEHEH ECKA
              HE OKABAET MEHEH BETA. BOMOHO,
              ATMEHHA  4678!./THE STAR IS BLUE;LIGHT VA-
              RIATIONS DURING 4D WERE NOT ACCOMPANIED BY
              COLOUR CHANGES. POSSIBLY AN ECLIPSING VARIA-
              BLE  4678!.
V 342  ARA    P>=140D.
V 344  ARA    P>=170D.
V 345  ARA    P>=180D.
V 349  ARA    MIN II 8.8.
V 355  ARA    P>220D.
V 356  ARA    P>170D.
V 357  ARA    P>=220D.
V 360  ARA    MIN II 13.8:, MIN II-MIN I=0.35P.
V 361  ARA    MIN II 13.6:.
V 362  ARA    MIN II 15.6:.
V 383  ARA    BEA 16.5M B K CEBEP/A STAR 16.5M IS
              CLOSE TO THE NORTH.
V 421  ARA    MIN II 15.1.
V 440  ARA    MIN II 14.5:.
V 444  ARA    MIN II 14.2.
V 454  ARA    MIN II 14.1.
V 480  ARA    MIN II 15.5:.
V 484  ARA    BOMOEH T RV (MIN=J.D. 2436760)./RV
              TYPE IS POSSIBLE (MIN=J.D. 2436760).
V 485  ARA    MIN II 14.8.
V 489  ARA    MIN II 11.9.
V 491  ARA    MIN II 11.9.
V 492  ARA    MIN II 14.5.
V 494  ARA    HE CKEH T RV./RV TYPE IS NOT EXCLUDED.
V 501  ARA    MIN II 13.8. OTMEEHA HA KAPTE  S 6114.
              /SHOWN IN THE CHART FOR S 6114.
V 535  ARA    MIN II 7.71. HEHEH EH B EMEHTAX:
              /NONLINEAR TERM IN THE ELEMENTS:-4.4D*10**-11*E**2.
V 536  ARA    MIN II MEETC/IS PRESENT. BOMOEH T EB.
              /EB TYPE IS POSSIBLE. P VAR.P=2.374101D
              (J.D. 2415000-22000); OCE/SINCE J.D. 2422000-
              - CM. TA./SEE TABLE.
V 539  ARA    VB A (B 9.22M, 12", 269G). MIN II 6.09, D=0.01P.
              OTMEEHA HA KAPTE  BV 1441=V 538 ARA.
              /SHOWN IN THE CHART FOR BV 1441=V 538 ARA.
V 544  ARA    BEA 14.5M SP./14.5M STAR SP.
V 609  ARA    OTMEEHA HA KAPTE  S 5867./SHOWN IN THE
              CHART FOR S 5867.
V 610  ARA    BOMOEH T EA./EA TYPE IS POSSIBLE.
V 613  ARA    VB (TECH NP CTHK/CLOSE NP COMPANION
              IS NSV 10198).
V 616  ARA    OK/DEEP MIN II.
V 620  ARA    MIN II BOMOEH/IS POSSIBLY PRESENT.
V 623  ARA    MIN II 14.5. BOMOEH OOBHH EPO.
              /TWICE SHORTER PERIOD IS POSSIBLE.
V 624  ARA    P>=220D.
V 625  ARA    P>=170D.
V 639  ARA    VI (NGC 6397). BEPOTHO, HE EH CKOEH.
              /PROBABLY NOT A CLUSTER MEMBER.
V 651  ARA    MIN II 15.3.
V 653  ARA    MIN II 12.6.
V 656  ARA    HE CKEH T EW./EW TYPE IS NOT EXCLUDED.
V 658  ARA    MIN II 16.0.
V 659  ARA    MIN II 14.4.
V 668  ARA    MIN II 13.8:.
V 675  ARA    P>=200D.
V 687  ARA    BOMOEH T RRC/RRC TYPE IS POSSIBLE.
V 700  ARA    MIN II 15.7.
V 702  ARA    MIN II 14.0.
V 704  ARA    MIN II 13.3.
V 705  ARA    MIN II 14.4. BOMOEH T RR./RR TYPE IS
              POSSIBLE.
V 716  ARA    HAEHO PABHOMEPHOE BEEHE ECKA HA
              HTEPBAE J.D. 2436689-36838. AMTA
              KOEAH, BEPOTHO, OE./MONOTONOUS
              BRIGHTENING DURING J.D. 2436689-36838 WAS
              FOUND. THE AMPLITUDE IS PROBABLY GREATER.
V 722  ARA    MIN II 10.3:.
V 728  ARA    MIN II 12.8.
V 732  ARA    HE CKEH T CEP./CEP TYPE IS NOT EXC-
              LUDED.
V 743  ARA    BOMOEH T RV./RV TYPE IS POSSIBLE.
V 781  ARA    MIN II 14.8:.
V 783  ARA    MIN II 13.9:.
V 785  ARA    MIN II 14.3.
V 787  ARA    BOMOEH T RV./RV TYPE IS POSSIBLE.
              MIN J.D. 2436756.
V 789  ARA    MIN II 14.8.
V 790  ARA    MIN II 14.8.
V 791  ARA    MIN II 13.0:.
V 792  ARA    MIN II 15.2:.
V 801  ARA    MXB 1636-53. OCAHE CEKTPA/DESCRIPTION
              OF THE SPECTRUM  1356!. B POKOOOCHOM
              OTECKOM OTOKE OTMEEHA MO C
              P-4H  AMTO O 40%  4944!./MODULATI-
              ON WITH P-4H AND THE AMPLITUDE UP TO 40% WAS
              FOUND IN THE BROAD BAND OPTICAL FLUX  4944!.
V 802  ARA    14.93-17.03 B.
V 808  ARA    BOMOEH T EW./EW TYPE IS POSSIBLE.
V 820  ARA    AHA OXA MIN. CHOE MAHTHOE OE.
               ATMEHHO-BOHA CCTEMA,  (TO BE-
              POTHEE) OOHA BPAAMC EPEMEHHM
              TA ACV./EPOCH OF MIN IS GIVEN. STRONG MAG-
              NETIC FIELD. EITHER AN=ECLIPSING BINARY OR (MO-
              RE PROBABLY) AN OBJECT SIMILAR TO ROTATING VARI-
              ABLES OF ACV TYPE.
V 821  ARA    4U 1658-48. HEOHA PEHTEHOBCKA CCTE-
              MA. LX/LOPT=3. HAAC KBAEPO-
              ECKE OTECKE KOEAH (P-20S) C O-
              HO AMTO 40%; PEKE BCK CO KA-
              O BPEMEH O 20MS, BO BPEM KOTOPX O-
              TOK MOET BOPACTAT B 2 PAA; MEHEHE
              ECKA HA 6M MEHEE EM A 2 MECA  4958!./
              UNUSUA1 X-RAY SYSTEM. QUASIPERIODIC OPTICAL
              VARIATIONS (P-20S) WITH TOTAL AMPLITUDE 40 PER-
              CENT, ABRUPT BURSTS ON-20 MS TIME SCALE LEA-
              DING TO TWO-FOLD FLUX INCREASE AND LIGHT CHANGES
              BY 6M DURING LESS THAN TWO MONTHS WERE OBSER-
              VED  4958!. LX/LOPT=3.
R      ARI    OH MCC/EMISSION.
T      ARI    P VAR. MAX=2417160+313.5D*E (J.D. 2404800-
              -17200); MAX=2434616+323.1D*E (J.D. 2419400-
              -34560). OCE/SINCE J.D. 2436560- CM. TA.
              /SEE TABLE. <P>=319.53D (J.D. 2404800- 44160).
              HOA/SOMETIMES A<1.5M.
U      ARI    SIO MAEP/MASER.
V      ARI    VR=-180 KM/C.
W      ARI    KAPT, AHHE B  2544, 6067!, HEBEPH./MAPS,
              GIVEN IN  2544, 6067! ARE WRONG.
X      ARI    B-V:+0.28, +0.56. P VAR. MAX=2420785.635+
              +0.6511248D*E (J.D. 2420460-33210)  3506!. OC-
              E/SINCE J.D. 2433210- CM. TA./SEE TABLE.
               FE/H!=-2.17.
RR     ARI    MIN II 6.75:; MIN II-MIN I=0.55P. OTOEKTPEC-
              KE HAEH PX ABTOPOB HE OTBEPAT
              EPEMEHHOCT ECKA/VARIABILITY IS NOT CONFIRMED
              BY OTHER AUTHORS' PHOTOELECTRIC OBSERVATIONS. V=
              =5.75.
RS     ARI    MIN II 11.0.
RU     ARI    OH MCC/EMISSION.
RV     ARI    B-V:+0.29, +0.44. 0.34P=<M-M=<0.53P. P1=0.07195D
               8137!; P2=0.27554D  7033!. MOMEHT PAX
              MAKCMMOB ECKA T/MOMENTS OF BRIGHTEST LIGHT
              MAXIMA T=2435066.400+0.31632996D*N  2290!.
RW     ARI    B-V:+0.35, +0.46. P VAR. MAX=2428183.324+
              +0.3543184D*E (J.D. 2428040-36700)  3188!. OC-
              E/SINCE J.D. 2440900 - CM. TA./SEE TABLE. CO-
              ACHO  6043! - ATMEHHA TA EA/ACCORDING TO
               6043! - EA TYPE: MIN I=2439384.97+3.1754D*E.
              OHE PEE MEHEH ECKA (11.47-
              -13.25 V)  8127! PECTABTC COMHTEHM.
              HE CKEHO, TO HAEHHE B  8127! ATMEH
               BEEHE ECKA RW ARI O'CHTC EPE-
              MEHHOCT OHO  COOBAHHX BE CPAB-
              HEH./TOTAL LIGHT RANGE (11.47-13.25 V)  8127!
              SEEMS DOUBTFUL. IT IS NOT EXCLUDED THAT THE ECLIP-
              SES AND LIGHT INCREASE OF RW ARI GIVEN IN  8127!
              ARE EXPLAINED BY VARIABILITY OF ONE OF COMPARISON
              STARS USED.
RX     ARI    D=0.02P. HA/DEPTH OF MIN II 0.10M.
SS     ARI    P VAR. MIN II 10.82:.
ST     ARI    P VAR. MAX=2427347+94.2D*E (1933-1939); MAX=
              =2429525+106.6D*E (1939-1942); MAX=2430588+
              +95.2D*E (1942-1946); MAX=2432118+100.0D*E
              (1946-1961). B TAE AH CPEHE EMEHT
              /MEAN ELEMENTS ARE GIVEN IN THE TABLE.
SX     ARI    B-V:-0.10, -0.12. AHA OXA MIN./EPOCH OF MIN
              IS GIVEN.
SZ     ARI    D=0.03P.
TT     ARI    PORB=0.137551D  8138!. KPOME MEHEH ECKA,
              XAPAKTEPHX  EPEMEHHX TA Z CAM, HA-
              ATC CHCOAHE KOEAH C AMTO
              OKOO 0.2M B, EPO KOTOPX MEHETC:/ALONG
              WITH LIGHT VARIATIONS TYPICAL FOR Z CAM VARIABLES
              THERE ARE SINUSOIDAL VARIATIONS WITH AMPLITUDE OF
              ABOUT 0.2M  B AND VARIABLE PERIOD: P=0.1329D
              (1961-62), P=0.1327D (1966)  4931!, P=0.1326D
              (1978)  4935!. HA CHCOAHE KOEAH HA-
              KABATC KBAEPOECKE KOEAH C
              KAM 8-20 MHT  AMTO O 0.2M, A TAK-
              E HEPABHE MEPAH O 0.1M A 1 MHT.
              /SINUSOIDAL VARIATIONS ARE SUPERIMPOSED BY QUASI-
              PERIODIC OSCILLATIONS UP TO 0.2M WITH 8-20 MINUTES
              CYCLE AND IRREGULAR FLICKERING UP TO 0.1M IN 1 MINUTE.
TU     ARI    P VAR. MAX=2420463.353+0.4716219D*E
              (J.D.2420463-34720). OCE/SINCE J.D.2436820-
              -CM. TA./SEE TABLE.
TV     ARI    P VAR.
TX     ARI    P VAR?
TY     ARI    OPMA KPBO ECKA MEHETC. PBEEHO CPE-
              HEE HAEHE EPOA/F ORM OF THE LIGHT CURVE VA-
              RIES. MEAN VALUE OF THE PERIOD IS GIVEN.
UV     ARI    OMHPET EPO BTOPOO OEPTOHA, AHH B
              TAE. HOA HAATC HAMEHTAH
              EPO P0=0.062D  EPO EPBOO OEPTOHA P1=
              =0.047D./THE SECOND OVERTONE PERIOD GIVEN IN THE
              TABLE IS DOMINATING. SOMETIMES THE FUNDAMENTAL
              PERIOD P0=0.062D AND THE FIRST OVERTONE PERIOD P1=
              =0.047D ARE OBSERVED.
UW     ARI    AMTA MEHETC/AMPLITUDE VARIES. B HTEP-
              BAE/IN THE INTERVAL J.D.2441581-693-CONST.
               7544!.
UX     ARI    T=2440133.766+6.43791D*E  6444!, E T-OXA
              COEHEH (KOMOHEHT G5 CA KOMOHEHTA KO).
              /WHERE T IS EPOCH OF CONJUNCTION (G5 COMPONENT
              IS BEHIND OF KO COMPONENT). ECK MEHETC BO-
              HOOPAHO C EPOOM, PMEPHO PABHM PORB
               6305!, HO AA PSI MHMMA ECKA, BCEH-
              HA OTHOCTEHO PBEEHHX BE EMEHTOB,
              CMEAETC C TEEHEM BPEMEH CEM OPA-
              OM:/BRIGHTNESS VARIES IN WAVES WITH A PERIOD-
              -PORB, BUT THE PHASE PSI OF LIGHT MINIMUM CALCULA-
              TED ACCORDING TO THE ELEMENTS GIVEN ABOVE CHANGES
              WITH TIME: PSI=0.1P (1972-1974), PSI=0.8P (1976), PSI=
              =0.7P (1977), PSI=0.6P (1978). CPEH ECK MEH-
              ETC, AMTA BOH MEHETC OT 0.04M O
              0.15M./MEAN BRIGHTNESS VARIES, AMPLITUDE OF THE
              WAVE VARIES FROM 0.04M UP TO 0.15M.
VW     ARI    BDS 1269 A (B 8.33M, 74", 31G). P2=0.089D. HEO-
              CTATOK METAOB. CTHK MEET HOPMAHOE CO-
              EPAHE METAOB./METAL DEFICIENCY. THE COM-
              PANION HAS NORMAL METAL ABUNDANCE.
VY     ARI    SB? AHA OXA MIN./EPOCH OF MIN IS GIVEN. HA-
              AETC TAKE BTOPOE KOEAHE ECKA:/SE-
              COND LIGHT VARIATION IS ALSO OBSERVED: MIN=
              =2442044.6+43.9D*E. HAAAC HEOA
              BCKA B AX U./A SMALL FLARE IN U BAND WAS
              OBSERVED.
GAMMA  ARI    VB A (B 4.65M, B 9 V, 7.9", 0G). AHA OXA MIN.
              /EPOCH OF MIN IS GIVEN.
R      AUR    VB A (B 8.6M, 48", 239G). P VAR  7165!; BOMOEH
              K 64.5A/CYCLE 64.5A IS POSSIBLE.
S      AUR    P VAR. B HAAE COPOKOBX OOB HAEO BEKA
              A CAA, MEHAC MAO  HEPABHO./IN
              THE EARLY FORTIES OF OUR CENTURY THE STAR WAS FAINT
              WITH SMALL AND IRREGULAR VARIATIONS.
T      AUR    MIN=2437614.0088+0.20437851D*E  8145!. P VAR?
              <V>=14.92, <B-V>=+0.28. BHE ATMEH-
              KTA ECKA. HA MIN-OT 0.10M O
              0.28M  3195!. CAA TMAHHOCT C BCOKO CTE-
              EH OHA./THERE ARE LIGHT FLUCTUATIONS
              BETWEEN THE ECLIPSES. DEPTHS OF MIN ARE 0.10M-
              -0.28M  3195!. FAINT NEBULA WITH HIGH DEGREE OF
              IONIZATION.
U      AUR    MAEP/H2O MASER.
Y      AUR    B-V:+0.70, +1.06.
Z      AUR    P VAR  7110!. MAX=2425580+110.76D*E
              (J.D.2416156-25580); MAX=2429888+113.35D*E
              (J.D.2425570-29900); MAX=2438292+135.55D*E
              (J.D.2429900-38300). P=110D (1965)  3196!. B
              1970 .-HEPABHE MEHEH  7338!/IN
              1970-IRREGULAR VARIATIONS  7338!. <V>=-165 KM/C;
              O TIO CEKTP M1  0806!/ACCORDING TO TIO BANDS
              THE SPECTRUM IS M1  0806!.
RS     AUR    P VAR.
RT     AUR    B-V:+0.39, +0.80.  A/H!=0.1. P VAR. MAX=
              =2433040.867+3.728365D*E (J.D.2417970-33100)
              OCE/SINCE J.D.2433100-CM. TA./SEE TABLE.
              DV VAR?
RU     AUR    MCC OH/EMISSION.
RV     AUR    CPEH BEHA, BOMOHO, MEHETC C =
              =10400D  1059!/MEAN MAGNITUDE PROBABLY VARIES
              WITH =10400D  1059!.
RW     AUR    VB A (B 12.5M, DM0E, 1", 2, 254G). CTHK, BO-
              MOHO, BCXBAET C AMTO 0.5M-0.7M
               3197, 3198!./THE COMPANION PROBABLY FLARES WITH
              AN AMPLITUDE 0.5M-0.7M  3197, 3198!. BOMOH
              EPO OCEBOO BPAEH 100D  7067!./POSSIBLE
              PERIOD OF AXIAL ROTATION IS 100D  7067!. MCC
              OH/EMISSION.
RX     AUR    B-V:+0.76, +1.18;  A/H!=-0.1, P VAR? HEHE-
              H EH:/NONLINEAR TERM:-0.70D*10**-6*E**2?
RZ     AUR    P VAR. MIN=2422616.498+3.010593D*E
              (J.D.2418000-26000); OCE/SINCE J.D.2426000-
              CM. TA./SEE TABLE.
SS     AUR    SB (P=0.1805939D  6103!). HOA HAAETC
              AHOMAHOE OBEEHE BE, KOA OBT-
              C CPABHTEHO ACTE  HEOE MAKCM-
              M ECKA. COACHO  8151! CPEH K 51.2D.
              /SOMETIMES ABNORMAL BEHAVIOUR OF THE STAR IS
              BEING OBSERVED WHEN COMPARATIVELY NUMEROUS AND
              SMALL LIGHT MAXIMA ARISE. ACCORDING TO  8151! THE
              MEAN CYCLE IS 51.2D.
SU     AUR    OPAET POK AP (P=3') C AB AUR C O-
              M COCTBEHHM BEHEM. CBAHA C HEO-
              O PKO TMAHHOCT. MCC OH./COMMON
              PROPER MOTION WITH AB AUR (P=3'). ASSOCIATED
              WITH A SMALL BRIGHT NEBULA. OH EMISSION.
SX     AUR    MIN II 8.87. COACHO  8153! P VAR/ACCORDING TO
               8153! P VAR: MIN I=2418218.7779+1.21007653D*E+
              +0.91D*10**-10*E**2.
SY     AUR    B-V:+0.92, +1.23.  A/H!=-0.3. P VAR  5661!.
              MAX=2436853.57+10.144330D*E (J.D.2417900-
              -32380). OCE/SINCE J.D.2432380-CM. TA.
              /SEE TABLE.
TT     AUR    MIN II 9.0.
TV     AUR    S 5/6-.
TW     AUR    CPEH BEHA MEHETC C P=1370D./MEAN
              MAGNITUDE VARIES WITH P=1370D.
TZ     AUR    B-V:+0.08, +0.48. DM=2.
UU     AUR    VB A (B 11M, 18", 222G).
UV     AUR    VB A (B 10.96M, B 9 V, 3.4", 4G). B CEKTPE PKE
              H  NEIII!   OIII!/BRIGHT LINES  NEIII! AND
               OIII! IN SPECTRUM.
UW     AUR    AHA OXA MIN/EPOCH OF MIN IS GIVEN.
UY     AUR    VB A (B 12M?, 0.8", 212G). MCC OH/EMISSION.
VW     AUR    VB (9.0M, 11.8M, 1.4", 332G, 1976).
VX     AUR    P VAR?
WW     AUR    MIN II 6.43. MIN II-MIN I=0.50P.
XX     AUR    MIN II 13.4.
YZ     AUR    B-V:+1.15, +1.72.  A/H!=-0.4.
ZZ     AUR    MIN II 11.1.
AB     AUR    CM./SEE SU AUR. OCAHE CEKTPA/SPECTRUM
              DESCRIPTION  4002!.
AE     AUR    CBAHA CO CBETO TMAHHOCT IC 405. A-
              ETC OT ACCOA ORI OB 1 CO CKOPOCT
              106 KM/C/CONNECTED WITH THE BRIGHT NEBULA IC
              405. THE MOTION IS DIRECTED AWAY FROM ORI OB 1
              ASSOCIATION WITH THE VELOCITY 106 KM/S.
AG     AUR    O TIO CEKTP M3  0806!/ACCORDING TO TIO BANDS
              THE SPECTRUM IS M3  0806!.
AH     AUR    MIN II 10.70. P VAR.
AK     AUR    VB B (A=BD+31G1370, 8.3M; B 82", 26G). B-V:
              +0.18.
AM     AUR    MIN II 11.0. P VAR: MIN I=2417617.2+13.6182D*E
              (J.D.2413500-19500)  0608!; OCE/SINCE
              J.D.2425400-CM. TA./SEE TABLE.
AN     AUR    B-V:+1.06, +1.48.  A/H!=-0.2.
AO     AUR    B-V:+0.86, +1.27.
AP     AUR    MIN II 11.2. P VAR: MIN I=2423080.505+
              +0.5692965D*E (J.D.2423080-35000). OCE/
              SINCE J.D.2435000-CM. TA./SEE TABLE.
AQ     AUR    OPMA KPBO ECKA/LIGHT CURVE SHAPE VAR?
AR     AUR    MIN II 6.70. MIN II-MIN I=0.50004P. P VAR: MIN I=
              =2427887.7217+4.13467D*E (J.D.2427800-
              -29500)  4999!. OCE/SINCE J.D.2438400-TA-
              HE EMEHT C KBAPATHM EHOM:/ELE-
              MENTS IN THE TABLE WITH AN ADDITIONAL NONLINEAR
              TERM:-2.2D*10**-8*E**2.
AZ     AUR    TECH CTHK/CLOSE COMPANION 16.3M B.
BC     AUR    MIN II 11.7.
BF     AUR    MIN II 9.49. P VAR. MIN I=2434455.3872+
              +1.583217D*E (J.D.2411760-34455)  5038!. OCE
              /SINCE J.D.2434455-CM. TA./SEE TABLE. OA
              PA HAEH OHAKOBO XOPOO PECTAB-
              TC OPMO/THE TWO SETS OF OBSERVATIONS ARE
              EQUALLY WELL REPRESENTED BY THE FORMULA: MIN I=
              =2440628.3643+1.5832212D*E+1.7D*10**-10*E**2
               8160!.
BH     AUR    P VAR. MAX=2437352.461+0.45608821D*E
              (J.D.2417260-42750)  7806!. OCE/SINCE
              J.D.2442750-CM. TA./SEE TABLE.
BK     AUR    B-V:+0.86, +1.26.
CI     AUR    HA/DEPTH OF MIN II 0.05M. P VAR. MIN I=
              =2439414.573+1.869984D*E+0.020D*10**-8*E**2
              (J.D.2425560-42045). EMEHT, AHHE B TA-
              E, CPABEB B HTEPBAE J.D.2439052-
              -40654/ELEMENTS GIVEN IN THE TABLE REPRESENT
              OBSERVATIONS IN THE INTERVAL J.D.2439052-40654.
CL     AUR    MIN II 12.3; MIN II-MIN I=0.45P; DII=0.13P. P VAR?
              MIN I=2432967.262+1.2443666D*E (J.D.2416900-
              -32967)  0608!. OCE/SINCE J.D.2432967-CM.
              TA./SEE TABLE.
CO     AUR    B TAE AH EPO 1-O OEPTOHA; EPO 2-O
              OEPTOHA P=1.4255D./THE FIRST OVERTONE PERIOD IS
              GIVEN IN THE TABLE; THE SECOND OVERTONE P=1.4255D.
CQ     AUR    B-V:+0.86, +1.07; MIN II 9.14:; MIN II-MIN I=
              =0.52P:; D=0.096P. P VAR. KBAPATH EH:/NON-
              LINEAR TERM:+3.78D*10**-7*E**2.
CY     AUR     A/H!=-0.3.
DV     AUR    P VAR. MAX=2426015+198.0D*E (J.D.2426014-
              -27400)  0332!. OCE/SINCE J.D.2439940-CM.
              TA./SEE TABLE.
EI     AUR    MIN II 15.0.
EM     AUR    MIN II 11.7.
EO     AUR    MIN II 7.89.
EP     AUR    MIN II 10.9. P VAR?
ER     AUR     A/H!=-1.1. P VAR? MAX=2432951.54+15.69073D*E
              (1949-1950)  1059!. B HTEPBAE/IN THE INTERVAL
              J.D.2443428-874-CM. TA./SEE TABLE.
EW     AUR     A/H!=-0.6.
FF     AUR     A/H!=-0.3.
FN     AUR    MIN II 12.3. P VAR?
FP     AUR    D=0.080P.
FR     AUR    MIN II 13.0.
FZ     AUR    D=0.40D.
GI     AUR    MIN II 11.7.
GK     AUR    MIN II 14.0; MIN II-MIN I=0.62P.
GO     AUR    P VAR. MAX=2426071+292.1D*E (J.D.2425505-
              -31325); MAX=2432205+301.2D*E (J.D.2432805-
              -36120)  3211!. OCE/SINCE J.D.2436990-CM.
              TA./SEE TABLE.
GY     AUR    MIN II 13.3.
HL     AUR    MIN II 11.0.
HN     AUR    B CKOEH/IN THE CLUSTER NGC 1664. KOEAHE
              C P1=165D: HAKABAETC HA KOEAHE C P2=
              =1400D:/LIGHT VARIATIONS WITH P2=1400D: ARE
              SUPERIMPOSED BY VARIATIONS WITH P1=165D:.
HP     AUR    MIN II 11.28; MIN II-MIN I=0.502P. P VAR. MIN I=
              =2427445.400+1.4228180D*E (J.D.2427445-
              -42683); OCE/SINCE J.D.2442712-CM. TA.
              /SEE TABLE.
HR     AUR    AHA OXA MIN/EPOCH OF MIN IS GIVEN.
HS     AUR    MIN II 11.2. HAEHE EPOA, AHHOE B  2619!
              CEET BOT, TAK KAK CCTEMA COCTOT 
              BX OHAKOBX KOMOHEHTOB  8164!/THE VA-
              LUE OF PERIOD GIVEN IN  2619! MUST BE DOUBLED AS
              THE SYSTEM CONSISTS OF TWO EQUAL COMPONENTS
               8164!.
HU     AUR    MIN II 12.4.
HW     AUR    MIN II 12.6.
HZ     AUR    HOA HAAETC TAKE KOPOTKOEPOEC-
              KE MEHEH VR C AMTE 3 KM/C  ECKA
              U C AMTE 0.02M./SOMETIMES SHORT PERIOD
              VARIATIONS OF VR WITH THE AMPLITUDE 3 KM/S AND OF
              BRIGHTNESS IN U WITH THE AMPLITUDE 0.02M ARE ALSO
              OBSERVED. MAX VR=2439454.900+0.073502D*E
               5259!. P (DU)=0.07396D  4818!.
II     AUR    MIN II 15.0:.
IM     AUR    MIN II 8.05:.
IQ     AUR    AHA OXA MIN./EPOCH OF MIN IS GIVEN.
IS     AUR    VB. AH PEE MEHEH CMMAPHOO ECKA.
              KAKO KOMOHEHT MEHETC, HEBECTHO/THE
              RANGE OF COMBINED BRIGHTNESS VARIATION IS GIVEN.
              IT IS NOT KNOWN WHICH OF THE COMPONENTS VARIES.
IU     AUR    P VAR. EMEHT COEPAT TPET EH:/THERE
              IS AN ADDITIONAL PERIODIC TERM IN THE ELEMENTS:
              -0.00627D*SIN (2.221G*E+15G). OTHOEHE -
              H MIN II K HE MIN I PABHO 0.78. HAAET-
              C BEKOBOE BEEHE H OOX MHM-
              MOB. HA MIN I BOPACTAET HA 0.016M B O.
              B TAE AH PEE MEHEH ECKA 
              1979.0 (MIN II 8.69). HAKOEHE OPT, BCE-
              CTBE PEECC OPT OT TPETEO TEA, BO-
              PACTAET HA 0.5G B O  5181!. OCAHE CEKTPA
               8166!./THE RATIO OF MIN II DEPTH TO MIN I DEPTH
              IS 0.78. THERE IS SECULAR DEEPENING OF BOTH MINI-
              MA. THE DEPTH OF MIN I INCREASES BY 0.016M PER
              YEAR. THE RANGE OF LIGHT VARIATION IN THE TABLE IS
              GIVEN FOR 1979.0 (MIN II 8.69). ORBITAL INCLINATION
              IS INCREASING BY 0.5G PER YEAR  5181! DUE TO ORBI-
              TAL PRECESSION CAUSED BY A THIRD BODY. SPECTRUM
              DESCRIPTION  8166!.
KO     AUR    MIN II 11.2.
KR     AUR    <B-V>=+0.10, <U-B>=-0.95. SB (P=0.1628D
               9045!). OCAHE CEKTPA/SPECTRUM DESCRIPTION
               8169, 8170!. POKE MCCOHHE H BOO-
              POA/WIDE HYDROGEN EMISSION LINES. POO-
              TEHE MAKCMM  MHMM, EC O-
              AM, HA KOTOPE HAKABATC CTPE ME-
              HEH ECKA HA 1-2M A H  ECTK HE 
              HA 0.5M A ECTK CEKH  8168, 8170!. CTO-
              HK MKOO PEHTEHOBCKOO EH  5191!.
              /LONG MAXIMA AND MINIMA LASTING FOR YEARS ARE
              SUPERIMPOSED BY RAPID LIGHT VARIATIONS BY 1-2M
              IN SEVERAL DAYS OR FORTNIGHTS AND BY 0.5M IN DO-
              ZENS OF SECONDS  8168, 8170!. THE SOURCE OF SOFT
              X-RAYS  5191!.
KS     AUR    VB A ( 12.5M, 5", 94G).
KV     AUR    HA OCKE BOH C KOM OKOO 750D HOA
              HAKABATC CPABHTEHO CTPE KOEA-
              H./FLAT WAVES WITH A CYCLE ABOUT 750D ARE SO-
              METIMES SUPERIMPOSED BY COMPARATIVELY RAPID FLUC-
              TUATIONS.
KW     AUR    VB A (B 11.0M, 11", 1, 352G, 1909; C 7.99M, 14.5",
              226G, 1923); SB 1 (P=3.788568D). CPEH ECK
              MEHETC C EPOOM OPTAHOO BEH.
              /MEAN LIGHT LEVEL VARIES SYNCHRONOUSLY WITH ORBI-
              TAL MOTION. HAP C OCHOBHM EPOOM CA-
               HAAETC EE BA EPOA HEPAAHO
              CA:/BESIDES MAIN PULSATIONAL PERIOD THERE
              ARE TWO MORE PERIODS OF NONRADIAL PULSATION:
              P1=0.096533D, P2=0.088243D.
KX     AUR    B TMAHHOCT IC 405/IN THE IC 405 NEBULA.
KY     AUR    CM./SEE KX AUR.
LY     AUR    VB A (B 9.1M, 0.6", 249G, 1958). MIN II 7.26; D=
              =0.017P.
MR     AUR    MIN II 15.5.
MT     AUR    D=0.02P.
NP     AUR    P VAR. OCE/SINCE J.D.2437720-CM. TA./SEE
              TABLE.
NU     AUR    EKT AKO/BLAZHKO EFFECT. =179D:.
NV     AUR    MAEP/OH, SIO, H2O MASER.
NW     AUR    B PAOHE CKOEH/IN THE REGION OF THE NGC 1893.
              MIN II 14.7. COACHO  7160!, HE APECTPPOBA-
              HO H OHOO MHMMA BO BPEM BAHX
              HAEH, OKPBX BA BCE A./AC-
              CORDING TO  7160! NO MINIMUM WAS RECORDED DURING
              VISUAL OBSERVATIONS COVERING TWICE ALL PHASES.
NX     AUR    B CKOEH/IN THE CLUSTER NGC 1893.
OP     AUR    B CKOEH/IN THE CLUSTER STOCK 8.
OX     AUR    VB A (B 10.0M, 22.4", 224G). P1=0.115442D. BO-
              MOHO MEHEHE CPEHEO ECKA./MEAN BRIGHTNESS
              PROBABLY VARIES.
PY     AUR    BOMOHO, EEA./POSSIBLY A CEPHEID.
QR     AUR    AHA OXA MIN./EPOCH OF MIN IS GIVEN.
QY     AUR    SB.
V348   AUR    VB A (B 13.43M, 24", 44G).
V353   AUR    B TEEHE HECKOKX ECTET ECK BOPA-
              CTA HA-0.06M B O. BOMOHO, BOHKAA
              AHETAPHA TMAHHOCT./DURING SEVERAL DECA-
              DES THE STAR BRIGHTENED BY-0.06M IN A YEAR. POS-
              SIBLY A PLANETARY NEBULA IN THE PROCESS OF FORMA-
              TION.
V358   AUR    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              NGC 2099.
BETA   AUR    VB A (B 14.1M, 13", 174G). MIN II 1.98.
EPSILO AUR    VB A (B 14.0M, 21", 224G). D=0.037P. OOP -
              ECKX OCOEHHOCTE CCTEM  2041, 2042, 3070,
              3216, 3217, 8174!. CEKTP, BOMOHO, MEHETC
              AE BHE ATMEH. ATMEH, O-BMOM, O-
              COBEH AO-EBM CKOM, OKPAM
              OP CTHK. ECK CTBAET ECKE
              KTA C AMTO O 0.24M  KOM OKO-
              O 110D  2040!, ATPHE BBEHE BOMO-
              HOO MIN II. OOH K HAEH B MEHEHX
              VR./SURVEY OF THE PHYSICAL PROPERTIES OF THE SYS-
              TEM  2041, 2042, 3070, 3216, 3217, 8174!. THE
              SPECTRUM PROBABLY VARIES EVEN OUTSIDE ECLIPSES.
              THE ECLIPSES ARE PROBABLY DUE TO A DISK OF GAS
              AND DUST SURROUNDING THE HOT COMPANION. THE
              BRIGHTNESS HAS PHYSICAL FLUCTUATIONS WITH THE AMP-
              LITUDE UP TO 0.24M AND THE CYCLE ABOUT 110D  2040!
              WHICH HINDER REVEALING THE POSSIBLE MIN II. SIMI-
              LAR CYCLE WAS DISCOVERED ALSO IN THE FLUCTUATIONS
              OF VR.
DZETA  AUR    PEE MEHEH ECKA CHO ABCT OT LAMBDA:
              /RANGE OF LIGHT VARIATION STRONGLY DEPENDS ON LAMBDA:
              4.98-5.53 B, 5.36-7.33 U. D=0.039P VAR:
              37.58D<=D<=38.07D  5486!. KTA ECKA K-
              BE HA 0.05M  5539!./LIGHT FLUCTUATIONS OF
              K-STAR BY 0.05M  5539!.
TETA   AUR    VB A (B 7.5M, 2", 8, 331G, 1924). COACHO  4034! EP-
              O MEHEH MAHTHOO O 3.618D./ACCORDING TO
               4034! THE PERIOD OF MAGNETIC FIELD VARIATION IS
              3.618D.
U      BOO    DM VAR (OT/FROM 0.9M O/TO 2.4M).
V      BOO    P VAR. A CHO MEHETC./A STRONGLY VARIES.
W      BOO    COACHO/ACCORDING TO  6994!, P=30D+-.
Z      BOO    H2O MAEP/MASER.
RS     BOO    DS=2. P VAR. O/BEFORE J.D.2435000 MAX=
              =2418115.5867+0.37733691D*E; OCE/SINCE
              J.D.2435000-CM. TA./SEE TABLE. MEHEH
              BCOT MAKCMMOB/CHANGES OF THE HEIGHT OF MA-
              XIMA: MAX (MHMAHA BCOTA/MINIMAL HEIGHT)=
              =J.D.2442500+533D*E; BOMOEH OEE KOPOT-
              K K MEHEH:/A SHORTER CYCLE OF CHANGES
              IS POSSIBLE: P-58-62D  4832!.
RU     BOO    B-V:+0.09, +0.44.
RX     BOO    H2O, SIO, OH MAEP/MASER.
SS     BOO    HA/DEPTH OF MIN II 0.1M.
ST     BOO    P VAR. MAX=2439236.032+0.6222968D*E (1966-
              -1974). CPEHE EMEHT/MEAN ELEMENTS
              1911-1974-CM. TA./SEE TABLE. EKT
              AKO/BLAZHKO EFFECT: MIN (O-C)=2442203+
              +284D*N. DS=11.
SU     BOO    D=0.032P. MIN II 12.04. P VAR.
SV     BOO    B-V:+0.17, +0.44. P VAR?
SW     BOO    B-V:+0.09, +0.39. P VAR. O/BEFORE J.D.2426500
              MAX=2421840.295+0.5134948D*E  2008, 2011!.
              OCE/SINCE 1960-CM. TA./SEE TABLE. BTO-
              PHOE KOEAHE/SECONDARY OSCILLATION: MAX
              (BCOTA/HEIGHT OF MAX)=2441037.33+12.997D*E.
              COACHO  4833!, ECK B MAX MEHETC ME
              10.5  11.6 V./ACCORDING TO  4833!, THE MAGNITU-
              DE IN MAX VARIES BETWEEN 10.5 AND 11.6 V.
SZ     BOO    P VAR?
TU     BOO    MIN II 12.4.
TV     BOO    B-V:+0.10, +0.22.  FE/H!=-2.42. EKT A-
              KO/BLAZHKO EFFECT, =16.14D  7116!.
TW     BOO    B-V:+0.11, +0.40. DS=12. P VAR. O/BEFORE
              J.D.2426890 MAX=2420340.551+0.53227557D*E;
              OCE/SINCE J.D.2426890-CM. TA./SEE TABLE.
TY     BOO    MIN II 11.35.P VAR.
TZ     BOO    MIN II 10.82 (VAR). DII=0.09P. P VAR. MHMM
              MEHTC B HE OT 10.8 O 11.0 V C P-
              -3.5 ET; BPEMEHAM MIN II E, EM MIN I.
              MEHTC  PE APAMETP OPM KPBO
              ECKA. B-1960 EPO MEHC CKAKOM;
              OTMEAC PE MEHEH EPOA./DEPTHS
              OF MINIMA VARY FROM 10.8 TO 11.0 V WITH P-
              -3.5 YRS; SOMETIMES MIN II IS DEEPER THAN MIN I.
              SOME OTHER PARAMETERS OF THE SHAPE OF LIGHT CUR-
              VE ARE ALSO VARIABLE. IN-1960 THE PERIOD CHAN-
              GED ABRUPTLY; OTHER PERIOD VARIATIONS WERE ALSO
              NOTED.
UU     BOO    B-V:+0.03, +0.44. P VAR. MEHEHE EPOA/
              /PERIOD CHANGE-J.D.2432700  3230!. O TOO
              /EARLIER MAX=2424967.310+0.45690626D*E  3229!.
UW     BOO    MIN II 10.5.
UX     BOO    COACHO/ACCORDING TO  2136!, DM-0.5M PG,
              EW?
UY     BOO    DS=12.6. P, DM VAR. O/BEFORE J.D.2425500
              MAX=2411459.819+0.6508552D*E; MAX=
              =2425688.836+0.6507849D*E (J.D.2425500-
              -28670)  1702!; MAX=2432306.759+0.650799D*E
              (J.D.2428670-32300)  2431!. OCE/SINCE
              J.D.2435900-CM. TA./SEE TABLE.
VW     BOO    MIN II 10.93. P VAR. KBAPATH EH:/NONLI-
              NEAR TERM:-0.084D*10**-9*(E-7500)**2.
WY     BOO    BOMOHO/POSSIBLY P=90D.
XY     BOO    MIN II 10.61. P VAR.
YZ     BOO    DS=0. DM VAR, OPMA KPBO ECKA MEHETC
              /THE SHAPE OF THE LIGHT CURVE VARIES  8186!.
ZZ     BOO    MIN II 7.44. BOMOH PAOCTOHK/POSSIB-
              LE RADIO SOURCE.
AC     BOO    MIN II 10.55. P VAR? H MIN  POBH MAX
              MEHTC./DEPTH OF MINIMA AND LEVEL OF MAXIMA
              ARE VARIABLE.
AD     BOO    MIN II 9.9.
AE     BOO    P VAR. (K-B)2=0.01.
AG     BOO    BOMOEH EKT AKO./BLAZHKO EFFECT IS
              POSSIBLE.
AK     BOO    MIN II 16.3.
AO     BOO    P VAR. AHA CPEH BEHA EPOA./MEAN PE-
              RIOD IS GIVEN.
AR     BOO    MIN II 14.5. P VAR.
AS     BOO    CM./SEE AG BOO.
BD     BOO    CM./SEE AG BOO.
BE     BOO    B MAKCMME ECKA HAAETC PAPOC TO-
              EK; P VAR?  5264!. BOMOHO, CTHH EP-
              O BETC COPEHHM KAAHHOM B TA-
              E./SCATTER IN THE LIGHT CURVE NEAR MAX LIGHT;
              P VAR?  5264!. THE VALUE OF THE PERIOD IN THE
              TABLE MAY BE SPURIOUS.
BG     BOO    MIN II 14.3.
BI     BOO    B OACT APOBOO CKOEH/IN THE REGION OF
              THE GLOBULAR CLUSTER NGC 5466.
BK     BOO    MIN II 15.3.
BL     BOO    V 19 (NGC 5466). B-V:+0.12, +0.25.  FE/H!=
              =-1.35. "AHOMAHA EEA". EH CKOEH
              O VR./"ANOMALOUS CEPHEID". RADIAL VELOCITY
              CLUSTER MEMBER.
BN     BOO    CM./SEE BI BOO.
BO     BOO    OPMA KPBO ECKA MEHETC: BEHA B MAX-OT
              14.5 O 15.0./THE SHAPE OF THE LIGHT CURVE VARI-
              ES: MAGNITUDE IN MAX-FROM 14.5 TO 15.0.
BP     BOO    5.51 V.
BR     BOO    PACCEHE TOEK OKOO CPEHE KPBO ECKA,
              BOMOHO, CBETECTBET O HEOXOMOCT
              TOHEH EPOA./THE MEAN LIGHT CURVE SHOWS
              SCATTER WHICH MAY EVIDENCE FOR THE NECESSITY TO
              IMPROVE THE PERIOD.
BU     BOO    CM./SEE AO BOO. CPEH KPB ECKA OCT-
              POT HE AETC./THE MEAN LIGHT CURVE COULD
              NOT BE OBTAINED.
BW     BOO    MIN II 7.17. MIN II-MIN I=0.450P. DII=0.06P. SB 1.
BX     BOO    VB A (B 10.6M, 36", 156G). P VAR. O PM AH-
              HM/ACCORDING TO OTHER SOURCES: MIN=244076730+
              +0.741285D*E  7955!; MIN=2440767.26+0.6080722D*E
               5054!.
CC     BOO    BEA HE KPACHA./THE STAR IN NOT RED.
CD     BOO    CM./SEE CC BOO.
CK     BOO    MIN II 9.23.
CP     BOO    P>0.125D.
GAMMA  BOO    VB A (B 12.5M, 33", 111G, 1925). DM VAR. O -
              EBM CKOPOCTM P=0.25D+-0.02D  4914!./RADIAL
              VELOCITY VARIES WITH P=0.25D+-0.02D  4914!.
KAPPA* *2     BOO ADS 9173 A (B=KAPPA**1 BOO, 6.69M, SB, F2V, 13",
236G).
              COACHO/ACCORDING TO  7015!, P=0.0668D (20).
              EPO EH/BEAT PERIOD-16D  6086, 7015!.
KSI    BOO    ADS 9413 AB (4.7M, G8V; 6.6M, K4V; A=4.884",
              P=149.95A). B CEKTPE G8V BHA H LII
              LAMBDA 6708. B OOX CEKTPAX OTMEATC PHAK
              XPOMOCEPHO AKTBHOCT, MCC H  K CAII.
              MCTOHK MKOO PEHTEHOBCKOO EH.
              EPEMEHHM, BEPOTHO, BETC KOMOHEHT
              A  3873!, XOT  KOMOHEHTA B HAAETC E-
              PEMEHHOCT MCC H  K CA II C KOM 10-
              -11 ET./LII LAMBDA 6708 LINE IS PRESENT IN THE G8V
              SPECTRUM. BOTH SPECTRA SHOW MANIFESTATIONS OF
              CHROMOSPHERIC ACTIVITY, EMISSIONS OF H AND
              K CA II. SOFT X-RAY SOURCE. PROBABLY IT IS COMPO-
              NENT A THAT IS VARIABLE, THOUGH VARIABILITY OF H
              AND K CAII EMISSION WITH THE CYCLE 10-11 YEARS
              IS OBSERVED FOR COMPONENT B.
I      BOO    ADS 9494 B (A 5.1M, G0; A=3.8", E=0.43, P=
              =225A). MIN II 6.29. P VAR. MIN=2434132.517+
              +0.267812271D*E+0.115242D*10**-9*E**2 (1916-
              1958)  3239!; MIN=2438513.4166+0.2678143D*E
              (1947-1967)  8191!; OCE/SINCE 1968-CM. TA.
              /SEE TABLE. OPOHE CCEOBAH MEHEH
              EPOA  5222, 7352, 7353, 8181!. BOMOH
              CKAKOOPAHE MEHEH EPOA P
              J.D.2423800, 29300, 32300, 35150. MEHETC
              TAKE OPMA KPBO ECKA  HA MIN II.
              COACHO  2020!, BOMOHA TAKE EPEMEHHOCT
              ADS 9494 A C AMTO O 0.09M./DETAILED
              STUDIES OF PERIOD CHANGES  5222, 7352, 7353,
              8181!. SUDDEN PERIOD CHANGES AT J.D.2423800,
              29300, 32300, 35150 ARE POSSIBLE. THE SHAPE OF
              THE LIGHT CURVE AND THE DEPTH OF MIN II ARE ALSO
              VARIABLE. ACCORDING TO  2020!, IT IS ALSO POSSIB-
              LE THAT ADS 9494 A IS VARIABLE, WITH THE AMPLITU-
              DE UP TO 0.09M.
S      CAE    <B-V>=+0.33. P<1D.
X      CAE    (K-B)2=0.22.
R      CAM    S 2/5: E. P VAR.
T      CAM    S 5/5 E.
U      CAM    HTEPEPPE/INTERFERING P1=435.45D, P2=
              =223.17D; P3=3000D  1053!.
V      CAM    H2O, SIO MAEP/MASER.
Y      CAM    EA/SD. SB 1. MIN II 10.60. P VAR. MIN=
              =2424434.5071+3.3054975D*E+0.1215D*
              *SIN (0.0543G*E+186.8G) (J.D.2411400-33300)  0978!;
              MIN=2437375.4923+3.3055069D*E+5.3D*10**-8*E**2
              (J.D.2437375-41000)  7166!; OCE/SINCE
              J.D.2440000-CM. TA./SEE TABLE. ABH
              KOMOHEHT-EPEMEHHA TA DSCTC  7166!
              C A<=0.05M B. COACHO  4192!, EPO CA-
              , BOMOHO, CHXPOHOBAH C OPTAHM
              BPAEHEM  COXPAHETC PAKTECK OCTOH-
              HM (0.066458D) B TEEHE TEHOO BPEMEH.
              /THE PRIMARY COMPONENT IS A DSCTC VARIABLE
               7166! WITH A<=0.05M B. ACCORDING TO  4192!, THE
              PULSATIONAL PERIOD IS POSSIBLY SYNCHRONIZED WITH
              THE ORBITAL MOTION AND REMAINS PRACTICALLY CONS-
              TANT (0.066458D) DURING A LONG TIME INTERVAL.
Z      CAM    SB 2. HHEE COEHEHE G-KOMOHEHTA/LOWER
              CONJUNCTION OF THE G COMPONENT T=2438470.841+
              +0.289840D*E 5365!. B EPO ME BCKA-
              M KPBA ECKA MOPETC CO CEKTPA-
              HM EMEHTAM  MEET OP HA AE 0.88P
               PAMT MIN HA AE 0.15P. ATMEH HE HA-
              ATC. BHE MAKCMMOB ECK MEPAET C
              DM O 0.5M  P-16S-18S. B MAKCMME ECKA
              KTA ECKA MA  5365, 4193!./OUTSIDE
              OUTBURSTS THE LIGHT CURVE IS MODULATED WITH SPECT-
              ROSCOPIC ELEMENTS AND HAS A SHOULDER AT THE PHA-
              SE 0.88P AND A BROAD, SHALLOW DIP AT THE PHASE
              0.15P. OUTSIDE MAXIMA FLICKERING UP TO 0.5M WITH
              P-16S-18S IS OBSERVED. DURING MAXIMA BRIGHT-
              NESS FLUCTUATIONS ARE SMALL  5365, 4193!.
RS     CAM    CPEH ECK MEHETC./MEAN BRIGHTNESS VARIES.
RU     CAM     A/H!=+0.9:. P VAR. MIN=2417610.1+22.187D*E (1908-
              -1917), MIN=2421315.3+22.121D*E (1917-1922),
              MIN=2423195.6+22.217D*E (1922-1931), MIN=
              =2426350.4+22.138D*E (1931-1951), MIN=
              =2433700.2 +22.162D*E (1951-1961), MIN=
              =2437356.9+22.055D*E (1961-1965)  3243!.
              HEOHA EPEMEHHA. OPMA KPBO ECKA
              MEHETC. O 1964-POKE MAX, PEKE MIN;
              DM MEHAC BBOE, BOMOHO, C KOM 5.1A
               3241!. OCE 1964-1966 DM PEKO MEHAC
              (O 0.4M-0.1M  MEHEE), KPBA ECKA CTAA
              CMMETPHO; CPEH ECK MEHETC B PEE-
              AX 0.3M B. EPO HEPEPHO MEHETC B PE-
              EAX 19.4D-23.5D. HAATC P KOE-
              AH, CMEHE P PA CO CBOM A-
               O 0.5P  4206!. CEKTP HEOEH, C CH-
              M OOCAM CN  CAM C2./UNUSUAL VARI-
              ABLE. THE SHAPE OF THE LIGHT CURVE VARIES. BEFO-
              RE 1964 BROAD MAXIMA AND SHARP MINIMA WERE
              OBSERVED; DM VARIED DY THE FACTOR  OF 2, WITH A
              POSSIBLE CYCLE 5.1A  3241!. AFTER 1964-1966
              DM DECREASED ABRIPTLY  (TO 0.4M-0.1M AND SMAL-
              LER), THE LIGHT CURVE BECAME SYMMETRIC; THE ME-
              AN LIGHT VARIES IN THE RANGE OF 0.3M B. THE PERI-
              OD VARIES IRREGULARY IN THE INTERVAL 19.4D-23.5D.
              GROUPS OF OSCILLATIONS ARE OBSERVED TO REPLACE
               ONE ANOTHER, WITH PHASE SHIFTS UP TO 0.5P  4206!.
              UNUSUAL SPECTRUM WITH INTENSE CN AND WEAK
              C2 BANDS.
RW     CAM     A/H!=+0.4. P VAR?
RX     CAM    B-V:+1.05, +1.48.  A/H!=0.
RY     CAM    BOMOHO/POSSIBLY P2=150.8D.
SS     CAM    D=0.06P. MIN II 10.35:. P VAR; KBAPATH EH:
              /NONLINEAR TERM: +2.04D*10**-9*E2.
SV     CAM    HA/DEPTH OF MIN II 0.15M:PG. P VAR. B -
              MEHEHX EPOA BOMOEH K 50A  3371!.
              EMEHT B TAE ECTBT OCE 1967.5.
              /A CYCLE OF 50A MAY BE PRESENT IN PERIOD CHAN-
              GES. THE ELEMENTS IN THE TABLE ARE VALID SINCE
              1967.5.
SW     CAM    P VAR. O/BEFORE J.D.2437600 MAX=2434448+
              +254.2D E. OCE/SINCE J.D.2440000-CM.TA.
              /SEE TABLE.
SZ     CAM    EH PACCEHHOO CKOEH/MEMBER OF THE
              OPEN CLUSTER NGC 1502. ADS 2984 B (A=NSV
              1458 7.1M V; B 18", 304G). MIN II 7.24, D II=0.17P.
              P VAR. OCE/SINCE 1970-CM.TA./SEE TABLE;
              PAHEE/EARLIER MIN I=2427533.5191+2.6984166D*E
               2071!.
TU     CAM    MIN II 5.22.
TV     CAM     A/H!=-0.2.
TX     CAM    SIO MAEP/MASER.
UY     CAM    DM VAR (0.2M-0.5M V)  3528!.
UZ     CAM    P VAR? O/BEFORE J.D.2428700 MAX=2427992+
              +231.0D*E  0114!; OCE/SINCE J.D.2440000-
              -CM.TA./SEE TABLE.
WW     CAM    D=0.013D. MIN II 11.1.
XX     CAM    B HTEPBAE 1898-1980 HAAC EHCT-
              BEHH CMMETPH MIN J.D.2429632 PO-
              OTEHOCT 94D. ECK KTPET O
              0.2M A ECTK MHT  4271!. B CEKTPE-E-
              T BOOPOA, TOK EPOA. HEKOTO-
              PE ABTOP COMHEBATC B PHAEHOCT
              BE K T RCB, OTMEA, B ACTHOCT,
              OTCTCTBE K-TKA  5423, 5430!.
              /DURING 1898-1980 A SINGLE SYMMETRIC MIN
              J.D.2429632 WAS OBSERVED WHICH LASTED FOR
              94D. BRIGHTNESS FLUCTUATIONS UP TO 0.2M DURING
              SEVERAL DOZENS OF MINUTES   4271!. HYDROGEN
              DEFICIENCY AND CARBON EXCESS IN THE SPECTRUM.
              SOME AUTHORS EXPRESS DOUBT ABOUT THE STAR'S
              BEING AN RCB VARIABLE; IN PARTICULAR, THEY NOTE
              THE LACK OF IR EXCESS  5423, 5430!.
AB     CAM     A/H!=-0.1.
AD     CAM     A/H!=-1.0.
AE     CAM    MIN II 15.8.
AH     CAM    VB A (B 7"). P VAR. MAX=2433897.519+
              +0.3687404D*E (J.D.2427000-33897)  2305!.
              OCE/SINCE J.D.2438000-CM.TA./SEE TABLE.
              ECK B MAX MEHETC C BOMOHM KOM
              =46P  3506!./MAGNITUDE IN MAX VARIES WITH A
              POSSIBLE CYCLE =46 P  3506!.
AK     CAM    P VAR. MIN=2426393.180+2.226780D*E
              (J.D.2426390-36610)  2594!; OCE/SINCE
              J.D.2436000-CM.TA./SEE TABLE.
AS     CAM    D=0.009P. MIN II 8.97, DII=0.06P, MIN II-MIN I=
              =0.437P.
AT     CAM    MIN II 10.6.
AU     CAM    OEH KPACHA./VERY RED.
AV     CAM    D=0.04P.
AW     CAM    MIN II 8.36.
AX     CAM    OPOHE CEKTPAHE CCEOBAH/DETAI-
              LED SPECTRAL STUDIES  7191!,  7192!.
AY     CAM    MIN II 10.23, DII=0.12P, DII=0.02P. COACHO
               3260!, CEKTP A5./ACCORDING TO  3260!, THE
              SPECTRUM IS A5.
AZ     CAM    MIN II 10.8.
BI     CAM    DM=0.9M PG.
BK     CAM    C 1912 O 1932 HAAC EPOECKE
              CEKTPAHE MEHEH (P=4.4A), PEKPATB-
              EC K 1937  4282!./DURING 1912-1932 PERIO-
              DIC (P=4.4A) SPECTRAL CHANGES WERE OBSERVED
              WHICH CAME TO AN END DY 1937  4282!.
BM     CAM    SB 1 (P=80.174469D; E=0.35). AHA OXA MIN
              ECKA./EPOCH OF MIN LIGHT IS GIVEN.
R      CNC    SIO MAEP/MASER.
S      CNC    B OACT CKOEH C/IN THE FIELD OF PRAE-
              SEPE (NGC 2632) CLUSTER. D=0.015P. MIN II 8.39.
              P VAR.
U      CNC    VB A (B 3"). B OACT CKOEH C./IN THE
              FIELD OF PRAESEPE (NGC 2632) CLUSTER.
V      CNC    S 0.5/6E. ADS 6763 A (B 13.5M, 10", 270G).
RS     CNC    P2=1700D. B CEKTPE-H TC./TC LINES ARE
              PRESENT IN THE SPECTRUM.
RT     CNC    P2-600D.
RU     CNC    D=0.035P. MIN II 10.21:, DII<=0.07P.
RW     CNC    P VAR. OCE/SINCE J.D.2437000-CM.TA./SEE
              TABLE. COACHO  2088!, MAX=2421339.380+
              +0.5471932D*E+0.57D*10**-9. (E-5800)**2+0.028D*
              COS 0.0215G* (E+2260)+F (PSI, HI), E OCEH
              EH PECTABET COO CMM BX KOPOTKO-
              EPOECKX KOEAH  AETC PAKAM
              B ABCMOCT OT A KAOO  KOEAH, TAK
              KAK OCHOBHOE KOEAHE (P=0.547D) MEHETC C
              1=29.9D  2=91.1D. BEHA B MAX MEHET-
              C OT 10.7M O 11.8M, B MIN-OT 12.3M O 12.6M.
              /ACCORDING TO  2088!, MAX=2421339.380+
              +0.5471932D*E+0.57D*10**-9* (E-5800)**2+0.028D*
              COS 0.0215G* (E+2260)+F (PSI, HI); HERE THE LAST TERM
              IS THE SUM OF TWO SHORT PERIOD OSCILLATIONS AND
              IS GIVEN IN GRAPHICAL FORM, SINCE THE MAIN PERIOD
              (0.547D) VARIES WITH 1=29.9D AND 2=91.1D.
              MAGNITUDE IN MAX VARIES FROM 10.7M TO 11.8M, IN
              MIN FROM 12.3M TO 12.6M.
RY     CNC    B OACT PACCEHHOO CKOEH NGC 2632
              (C), HE EH CKOEH./IN THE REGION OF THE
              OPEN CLUSTER NGC 2632 (PRAESEPE),  NON-MEMBER.
              B-V: +0.58, +1.05. P VAR. O/BEFORE J.D.2436000
              MIN=2429334.445+1.0929500D*E; OCE/SINCE
              J.D.2436000-CM.TA./SEE TABLE.
RZ     CNC    MIN II 9.21. D=0.015P:. KOMOHEHT CO-
              AH./ELLIPSOIDAL COMPONENTS.
SS     CNC    DS=1.2. P VAR?
SV     CNC    B-V: +0.10, +0.52.
SY     CNC    CTPE KBAEPOECKE KTA EC-
              KA, P-20S-34S  5959!. CCEOBAHE CEKTPA
               4286!./FLICKERING WITH P-20S-34S  5959!.
              SPECTRAL INVESTIGATION  4286!.
TT     CNC    (K-D)2=0.11. P VAR. O/BEFORE J.D.2430700
              MAX=J.D.2425647.452+0.5634445D*E  3506!. OC-
              E/SINCE J.D.2439800-CM.TA./SEE TABLE. -
              EKT AKO/BLAZHKO EFFECT, =89D  5271!.
TW     CNC    D=0.014P. HA/DEPTH OF MIN II 0.1M PG.
TX     CNC    EH PACCEHHOO CKOEH C/MEMBER OF THE
              OPEN CLUSTER PRAESEPE (NGC 2632). MIN II 10.32.
TY     CNC    D=0.013P. P VAR.
UU     CNC    MIN II 9.2, J.D. (MIN II) 2435608.5. SB 1. KPBA
              ECKA HECTAHA.CEKTPAHE CCEOBA-
              H  1881!,  3149!,  4289!./THE LIGHT CURVE IS UNS-
              TABLE. SPECTRAL STUDIES  1881!,  3149!,  4289!.
UV     CNC    B OACT CKOEH C/IN THE REGION OF THE
              PRAESEPE (NGC 2632) CLUSTER.
UZ     CNC    MIN II 11.4.
VY     CNC    MIN II 12.3:.
VZ     CNC    (K-D)2=0.32. HAATC EH BX KOEA-
              H. COACHO  2125!,  CEPEH BOCXOE
              BETB T (M)=J.D.2433631.84615+0.17836376D*E+
              +0.00193D SIN 2 PI PSI (M) -0.00371D COS 2 PI PSI (M), E
              AA EPOA EH PSI (M) BCETC OT E-
              MEHTOB T (M) =J.D.2433631.8421+0.716292D*E.
              CM.TAKE  2124!. CEKTPAHOE CCEOBAHE
               2126!./BEAT PHENOMENON FOR TWO OSCILLATIONS IS
              OBSERVED. ACCORDING TO  2125!, FOR THE MIDDLE OF
              THE ASCENDING BRANCH T (M) =2433631.84615+
              +0.17836376D*E+0.00193D SIN 2 PI PSI (M) -
              -0.00371D COS 2 PI PSI (M); HERE THE PHASE OF THE BEAT
              PERIOD PSI (M) IS COMPUTED WITH THE ELEMENTS T (M) =
              =J.D.2433631.8421+0.716292D*E. SEE ALSO  2124!.
              SPECTRAL INVESTIGATION  2126!.
WW     CNC    COACHO  7531!, EPO OCTOHEH C 1933. P
              MHMMOB BBSAG POTBOPET TAHM
              EMEHTAM./ACCORDING TO  7531!, THE PERIOD DO-
              ES NOT VARY SINCE 1933. A NUMBER OF MINIMA DY
              BBSAG CONTRADICT THE TABULATED ELEMENTS.
WX     CNC    MIN II 10.7.
WY     CNC    VB A (B 12.8M, -20", 0G). MIN II 9.60.
XX     CNC    CM./SEE UV CNC.
XZ     CNC    MIN II 10.2.
YY     CNC    COACHO  3263!, BEPOTHO, HEPABHA./AC-
              CORDING TO  3263!, THE STAR IS PROBABLY AN IRREGU-
              LAR VARIBLE.
YZ     CNC    B MAKCMME ECKA HAATC KOEAH C
              P=133.2M/OSCILLATIONS WITH P=133.2M ARE OBSER-
              VED IN MAXIMUM LIGHT  6249!.
ZZ     CNC    D=0.02P:.
AC     CNC    MIN II 14.7. <MAX>=14.5. ECK BHE ATMEH
              MEHETC B PEEAX 13.8-15.2 B. 3 OKX
              MHMMA HE OBETBOPT TAHM EMEH-
              TAM  4460!. HE CKEHA TOECTBEHHOCT C
              PEHTEHOBCKM CTOHKOM H 0857+13./THE BRIGHT-
              NESS OUTSIBE ECLIPSES VARIES IN THE RANGE 13.8-
              -15.2B. 3 DEEP MINIMA CONTRADICT THE TABULATED
              ELEMENTS  4460!. THE IDENTIFICATION WITH THE X-RAY
              SOURCE H 0857+13 IS NOT EXCLUDED.
AD     CNC    MIN II 13.4.
AH     CNC    EH PACCEHHOO CKOEH/MEMBER OF THE OPEN
              CLUSTER M 67 (NGC 2682). MIN II 13.68. KBAPAT-
              H EH:/NONLINEAR TERM: +1.56D*10**-10*E**2. BOMOH
              TAKE KECKE MEHEH EPOA (C PA-
              HM KAM)  4475!./CYCLIC PERIOD VARIATIONS
              (WITH DIFFERENT CYCLES) ARE ALSO POSSIBLE  4475!.
AO     CNC    MIN II 13.4.
AP     CNC    P VAR?
AU     CNC    BOMOH EH CKOEH C/POSSIBLE MEM-
              BER OF THE CLUSTER PRAESEPE (NGC 2632).
AV     CNC-AZ CNC CM./SEE AU CNC.
BB     CNC    DMU>6.0. CM./SEE AU CNC.
BC     CNC    DMU>4.0. CM./SEE AU CNC.
BD     CNC-BE CNC CM./SEE AU CNC.
BG     CNC-BH CNC CM./SEE AU CNC.
BI     CNC    EMEHT OPEE BHEP. AHA OXA MAX B
              OOCE U./THE ELEMENTS WERE DETERMINED DY
              WINZER. EPOCH OF MAX IN U BAND IS GIVEN.
BK     CNC    CM./SEE AU CNC.
BM     CNC    SB (P=585.4154D  6568!). B TAE AH E-
              MEHT  MOMEHTOB MAKCMMOB (B-V)./THE
              ELEMENTS IN THE TABLE REPRESENT THE MOMENTS OF
              MAXIMAL (B-V).
BN     CNC    EH CKOEH C/MEMBER OF THE CLUSTER PRA-
              ESEPE (NGC 2632).
BQ     CNC    SB CM./SEE BN CNC.
BR     CNC    VB A (B 14.2M, 30", 268G). CM./SEE BN CNC.
BS     CNC    CM./SEE BN CNC.
BT     CNC    CM./SEE BN CNC. HAKABATC KOEAH C
              PM EPOAM./OSCILLATIONS WITH OTHER PE-
              RIODS ARE SUPERIMPOSED.
BU     CNC    CM./SEE BN CNC. COACHO  4483!, P=0.071D HE
              OTBEPAETC, B PAHE HO HAATC
              P=0.0534D, P=0.059D  PE EPOHOCT.
              /ACCORDING TO  4483!, P=0.071D IS NOT CONFIRMED;
              DURING DIFFERENT NIGHTS P=0.0534D, P=0.059D AND
              SEVERAL OTHER PERIODICITIES WERE OBSERVED.
BV     CNC-BY CNC CM./SEE BN CNC.
BZ     CNC    SM>?SEE UV CNC.
CC     CNC    K/CYCLE<=90D.
CD     CNC    CM./SEE AU CNC.
CE     CNC-CH CNC CM./SEE UV CNC.
CI     CNC    CM./SEE AU CNC.
CK     CNC-CL CNC CM./SEE UV CNC.
CM     CNC-CN CNC CM./SEE AU CNC.
CO     CNC-CP CNC CM./SEE UV CNC.
CR     CNC-CS CNC CM./SEE UV CNC.
CU     CNC    G 9-8=G 40-25. VB A (B=CV CNC, 13", 347G),
              OEE MU/COMMON MU. B PAOHE CKOEH C,
              HE EH CKOEH./IN THE REGION OF PRAESEPE
              (NGC 2632) CLUSTER, NON-MEMBER.
CV     CNC    G 40-26. CM./SEE CU CNC.
CY     CNC    CM./SEE BN CNC.
CZ     CNC    KOOPHAT B  8354! OTHOCTC K PABHOEHCT-
              B 2000.0. /EQUINOX IN  8354! MUST BE 2000.0.
DD     CNC    CM./SEE UV CNC.
DF     CNC    CM./SEE UV CNC. BOMOHO, HE EH CKOEH
              /POSSIBLY NON-MEMBER.
DG     CNC    CM./SEE DF CNC.
DH     CNC-DI CNC CM./SEE AU CNC.
DL     CNC    VB. CM./SEE UV CNC.
DM     CNC    CM./SEE AU CNC.
DN     CNC-DP CNC CM./SEE UV CNC.
DQ     CNC    CM./SEE DF CNC.
DR     CNC    CM./SEE UV CNC.
DS     CNC    CM./SEE DF CNC.
DT     CNC-DU CNC CM./SEE UV CNC.
KAPPA  CNC    SB (P=6.39316D). B  4487! EPEMEHHOCT ECKA
              HE OTBEPAETC./IN  4487! THE LIGHT VARIABI-
              LITY WAS NOT CONFIRMED.
R      CVN    P VAR. MAX=2411768+325.4D*E (J.D.2411730-
              -26430)  1701!; MAX=2432074+332.8D*E
              (J.D.2426750-32100); OCE/SINCE J.D.2432100
              -CM.TA./SEE TABLE.
T      CVN    SRA? DM CHO MEHETC/STRONGLY VARIES.
U      CVN    MCC OH, H2O/EMISSION.
V      CVN    MAEP H2O, SIO/MASER.
W      CVN    B-V:+0.15, +0.42. P VAR. KBAPATH EH:/
              NONLINEAR TERM: -368*10**-13*E**2. DS=7.
Y      CVN    P2=2000D.
Z      CVN    B-V: +0.20, +0.33. P VAR. MAX=2413000.262+
              +0.6538236D*E (J.D.2413000-23170); MAX=
              =2423860.355+0.6539052D*E (J.D.2423860-
              -31800)  1702!; MAX=2432943.645+0.653824D*E
              (J.D.2431800-40200)  6457!. OCE/SINCE
              J.D.2438900-CM.TA./SEE TABLE. EKT
              AKO:/BLAZHKO EFFECT:MIN. AMP1.=2439176.12+
              +22.75D*E  3267!. AMTA MEHETC HA
              0.5M B, EPOECKE OTKOHEH OX MAX
              OT HEHX EMEHTOB OCTAT +-0.02D./AM-
              PLITUDE VARIES DY 0.5M B, EXTREMAL PERIODIC DE-
              VIATIONS  OF THE EPOCH OF MAX FROM LINEAR ELE-
              MENTS ARE +-0.02D. DS=8.
RR     CVN    B-V: +0.09, +0.45.  FE/H!=-1.33. OPMA KP-
              BO ECKA  DM MEHTC./THE LIGHT CUR-
              VE SHAPE AND DM VAR.
RS     CVN    MIN II 8.19; MIN II-MIN I=0.506P; D=0.033P.
              P VAR. KBAPATH EH:/NONLINEAR TERM:
              -1.00D*10**-8*E**2. HA KPBO ECKA BHE ATME-
              H HAAETC MPPEE BOHOOPAHOE
              BOMEHE C AMTO OT 0.09M O 0.20M 
              EPOOM 4.7917D, KM K OPTAHOM
               7209!. A 9.48 OA BOHA CMEAETC O AE
              HA EPO B HAPABEH MEHEH A  5800!.
              /WAVE-LIKE DISTORSION WITH THE AMPLITUDE FROM
              0.09M UP TO 0.20M AND WITH THE PERIOD 4.7917D CLO-
              SE TO THE ORBITAL ONE IS OBSERVED ON THE LIGHT
              CURVE OUT OF ECLIPSES  7209!. THE WAVE IS MIGRA-
              TING ON PHASE IN THE DIRECTION OF PHASE DECREASING
              WITH A MIGRATION PERIOD OF 9.48 YEARS  5800!.
RU     CVN    B-V: +0.10, +0.39. P VAR. MAX=2420227.338+
              +0.5732502D*E (J.D.2418801-29436)  5436!; MAX=
              =2420227.398+0.57324647D*E (J.D.2418979-
              -36665)  3271!; OCE/SINCE J.D.2434483-CM.
              TA./SEE TABLE.
RV     CVN    V 141 (M3/NGC 5272). HE EH CKOEH./NOT
              A MEMBER OF THE CLUSTER. MIN II 15.81.
RX     CVN    B-V: +0.17, +0.41. P VAR?
RZ     CVN    B-V: +0.12, +0.43. P VAR. MAX=2424621.489+
              +0.56740036D*E (J.D.2424620-31000)  0188!;
              MAX=2437823.433+0.5674174D*E (J.D.2434470-
              -37830); OCE/SINCE J.D.2438200-CM.TA.
              /SEE TABLE.
ST     CVN    P VAR?DS=4.8.
SV     CVN    P VAR. MAX=2427434.911+0.66805653D*E
              (J.D.2426000-32000)  0752!; OCE/SINCE
              J.D.2439500-CM.TA./SEE TABLE.
SW     CVN    P VAR. MAX=2431139.791+0.44164922D*E
              (J.D.2425640-32000)  0752!; OCE/SINCE
              J.D.2436200-CM.TA./SEE TABLE.
TX     CVN    SB 2 (P=70.8D)  4504!.
UU     CVN    B PAOHE APOBOO CKOEH/IN THE REGION OF
              THE GLOBULAR CLUSTER NGC 5466. P VAR. MAX=
              =2437817.312+0.5409589D*E (J.D.2436360-39945);
              OCE/SINCE J.D.2439945-CM.TA./SEE TABLE.
UV     CVN    B PAOHE APOBOO CKOEH NGC 5466. HE
              EH CKOEH./IN THE REGION OF GLOBULAR CLUSTER
              NGC 5466, NON-MEMBER. P VAR. MAX=2419446.156+
              +0.6316090D*E (J.D.2419440-34455); OCE/SIN-
              CE J.D.2434450-CM.TA./SEE TABLE.
UW     CVN    B PAOHE APOBOO CKOEH/IN THE REGION OF
              THE GLOBULAR CLUSTER NGC 5466.
UX     CVN    MIN II 11.94. U-B: -1.05, -0.99; B-V: -0.29,
              -0.23.
VV     CVN    MIN II 14.3:.
VW     CVN    MIN II 12.4. P VAR. MIN I=2435923.246+0.8499757D*E
              (J.D.2427900-36000); OCE/SINCE J.D.2435900-
              -CM.TA./SEE TABLE. HA KAPTE HE KAAHA. HA-
              XOTC B 6MM K AA  3MM K CEBEP OT
              BE CPABHEH C./THE VARIABLE IS NOT MAR-
              KED ON THE MAP. IT IS DY 6MM TO THE WEST AND
              3MM TO THE NORTH OF THE COMPARISON STAR C.
VZ     CVN    MIN II 9.54.
WW     CVN    BOMOHO HAE EKTA AKO./BLAZHKO
              EFFECT IS POSSIBLE.
WY     CVN    V 205 (M3/NGC 5272). EH CKOEH?/MEMBER
              OF THE CLUSTER? CM./SEE WW CVN.
WZ     CVN    V 206 (M3/NGC 5272). HE EH CKOEH? -
              EKT AKO./NON-MEMBER? BLAZHKO EFFECT.
XX     CVN    B PAOHE APOBOO CKOEH M3 (NGC 5272).
              EH CKOEH?/IN THE REGION OF M3 (NGC 5272)
              GLOBULAR CLUSTER. MEMBER OF THE CLUSTER?
YZ     CVN    D=0.055P,  HA MIN II/DEPTH OF MIN II 0.05M
              VIS.
AA     CVN     FE/H!=-1.78.
AD     CVN     FE/H!=-1.39.
AF     CVN     FE/H!=-1.19.
AG     CVN     FE/H!=-2.01.
AH     CVN     FE/H!=-2.01.
AI     CVN    PAAHE MTEPOECKE CA
              /RADIAL MULTIPERIOD PULSATIONS: P0=0.2085D,
              P1=0.1529D, P2=0.1259D, P3=0.1158D.
AK     CVN     FE/H!=-1.19.
AM     CVN    KPBA MEHEH ECKA-BOHA BOHA.
              BTOPH MHMM HOA CEAET. -
              HA MIN I TAKE MEHETC.B TAE AHA O-
              XA MIN I. P VAR; DP/DT=+0.012S/O. B TAE
              AH EMEHT  1978. ECK KTP-
              ET C KOM 115-120S, HOA HAAETC E-
              POHOCT C P=26.3S. BOMOHO, TECHA
              BOHA OPAEEHHA CCTEMA C AKKPE-
              OHHM CKOM  OPM THOM, COCTOA
               BX EX KAPKOB./THE LIGHT CURVE IS A
              DOUBLE WAVE. MIN II SOMETIMES DISAPPEARS. THE
              DEPTH OF MIN I CHANGES ALSO. EPOCH OF MIN I IS
              GIVEN IN THE TABLE. P VAR; DP/DT=+0.012S PER
              YEAR. ELEMENTS FOR 1978 ARE GIVEN IN THE TABLE.
              THE BRIGHTNESS FLUCTUATES WITH THE CYCLE OF
              115-120S, SOMETIMES THE PERIODICITY WITH P=
              =26.3S IS OBSERVED. PROBABLY IT IS A CLOSE BINA-
              RY SEMIDETACHED SYSTEM OF TWO WHITE DWARFS
              WITH AN ACCRETION DISK AND A HOT SPOT.
AN     CVN     FE/H!=-1.54.
AQ     CVN    OOHA BEAM OPOHTAHO BETB APO-
              BX CKOEH. HAAAC BCKA, B-
              AC 20 MHT./SIMILAR TO HORIZONTAL BRANCH
              STARS IN GLOBULAR CLUSTERS. A FLARE LASTING 20
              MINUTES WAS OBSERVED.
BF     CVN    G 123-75=G 164-32. VB A (B=G 164-31, 13.16M,
              DM 3.5E; 17", 225G). OTMEEH BCK B CM-
              MAPHOM ECKE CCTEM, DU O 0.95M./FLARES
              IN THE COMBINED LIGHT OF THE SYSTEM (DU UP TO
              0.95M) WERE OBSERVED.
BG     CVN    P1=1186S, P2=780S.
BH     CVN    SB. EKT OTPAEH/REFLECTION EFFECT DM=
              =0.013V.
BI     CVN    MIN II 10.70. P VAR?
A**2   CVN    VB A (B 5.60M, F0V, 19.6", 228G). AHA OXA
              MIN./EPOCH OF MIN IS GIVEN.
R      CMA    MIN II 5.78. P VAR  3280, 6314!. METC AHOMA-
               KPBO ECKA  3281, 3282!./THE STAR SHOWS
              ANOMALIES OF THE LIGHT CURVE  3281, 3282!.
V      CMA    VB B (A=CPD-31G1311, 9M4; B 16", 90G).
Z      CMA    MOH K-TOK. CEKTP OOOK. P
              H OKABAET PO TA P CYG. BEA
              HAXOTC B OATO ETAM TMAHHOCT.
              B BE HAAETC PK BCT T-
              MAHHOCT, ME HEPEPBH CEKTP, BE-
              POTHO, EHTH CEKTP CAMO BE./
              STRONG IR EXCESS. SHELL SPECTRUM. SEVERAL LINES
              SHOW P CYG PROFILES. THE STAR IS LOCATED IN A
              NEBULA RICH IN DETAILS. A BRIGHT WISP OF NEBU-
              LOSITY NEAR THE STAR  HAS CONTINUONS SPECTRUM,
              PROBABLY IDENTICAL TO THAT OF THE STAR  4002!.
RR     CMA    MIN II 13.1.
RT     CMA    MIN II 11.5. C ETOM OX   3283! BOMO-
              EH P=1.293745D./P=1.293745D IS POSSIBLE TA-
              KING INTO ACCOUNT THE EPOCH FROM  3283!.
RX     CMA    D=0.027P. MIN II 11.1. P VAR. B HTEPBAE/ DURING
              J.D.2441700-43000-CM.TA./SEE TABLE.
RZ     CMA    P VAR? OCE/SINCE J.D.2435500-CM.TA.
              /SEE TABLE.
SW     CMA    MIN II 9.9. MIN II =J.D.2426709.366; MIN II-MIN I=
              =0.316P.
SX     CMA    MIN II 10.3.
TU     CMA    MIN II 10.1.
UW     CMA    MIN II 5.25. AOBE OTOK, PACPAC
              AOBA OOOKA. MHMM ACCMETPH;
              HAATC PE HEPABHOCT KPBO
              ECKA. P CEKTPAHX H MET PO-
               TA P CYG. HAAETC EPEMEHHOCT PO-
              E H B ABCMOCT OT OPTAHO A-
              , A TAKE ( 7227!, O AHHM SANYAL) C XAPAK-
              TEPHM BPEMEHEM MEHEE 1**H./GASEOUS STREAMS,
              EXPANDING GASEOUS ENVELOPE. MINIMA ARE ASYM-
              METRIC; OTHER PECULIARITIES OF THE LIGHT ARE OBSER-
              VED. A NUMBER OF SPECTRAL LINES HAVE P CYG PRO-
              FILES. THE LINE PROFILES ARE OBSERVED TO VARY WITH
              THE PHASE OF THE ORBITAL PERIOD, AND ALSO ( 7227!,
              ACCORDING TO SANYAL) WITH CHARACTERISTIC TIME
              <1**H.
UX     CMA    MIN II 12.3.
VW     CMA    MIN II 9.1.
VY     CMA    ADS 6033 A (B 9.2M, 0.5", 168G; C 11.5M, 2.7", 291G;
              D 11M, 2.9", 347G, ...). H2O, OH, SIO MAEP/MASER.
              B-V: +2.3. B PAOHE MOOOO PACCEHHOO CKO-
              EH NGC 2362. B OTPAATEHO TMAHHOCT.
              CTHK MOT T ETAM TMAHHOCT; HE-
              KOTOPE  HX, BEPOTHO, EPEMEHH  2159,
              3287!. OKPEHA AOBO-EBO OOOKO 
              CKOM OBOO PAMEPA 0.45" (LAMBDA=5 MU M). C 1801
              HAAOC BEKOBOE OCAEHE ECKA. HA-
              ATC TAKE KECKE MEHEH ECKA C
              DM OT HECKOKX ECTX O 3M POOTE-
              HOCT OT 200D O 1900D. B CEKTPE-MCC-
              OHHE OOC TIO  SCO. CEKTPAHE CCE-
              OBAH  3287, 5282, 6133!./IN THE REGION OF THE
              YOUNG OPEN CLUSTER NGC 2362. EMBEDDED IN A
              REFLECTING NEBULA. THE COMPANIONS MAY BE DETA-
              ILS OF THE NEBULA;SOME OF THEM ARE PROBABLY VA-
              RIABLE  2159, 3287!. SURROUNDED BY AN ENVELOPE
              OF GAS AND DUST OR A DISK OF 0.45" (LAMBDA=5 MU M) ANGU-
              LAR SIZE. SECULAR DECREASE OF BRIGHTNESS SINCE
              1801. CYCLIC VARIATIONS OF BRIGHTNESS WITH DM
              FROM SEVERAL TENTHS OF A MAGNITUDE TO 3M ON TI-
              ME SCALE FROM 200D TO 1900D. TIO AND SCO EMIS-
              SION BANDS IN THE SPECTRUM. SPECTROSCOPIC STU-
              DIES  3287, 5282, 6133!.
WW     CMA    RR, MAX=2428570.09+0.499355D*E  0613!. CEP,
              MAX=2428146.6+5.7660D*E  0514!. TM EMEH-
              TAM POTBOPEAT 94 OTOPAECKX HA-
              EH EPEKCOBO  12 OTOEKTPECKX HA-
              EH PBHA  3288!./THESE SYSTEMS OF
              ELEMENTS ARE CONTRADICTED BY 94 PHOTOGRAPHIC
              OBSERVATIONS (ERLEKSOVA) AND 12 PHOTOELECTRIC
              OBSERVATIONS (IRWIN,   3288!).
XY     CMA    D=0.04P:.
ZZ     CMA    MIN II 13.0.
AE     CMA    D=0.02P:.
AN     CMA    D=0.02P:.
AO     CMA    B OACT PACCEHHOO CKOEH/ IN THE FIELD
              OF THE OPEN CLUSTER RUPRECHT 18.
AR     CMA    D=0.025P:.
AS     CMA    D=0.04P.
BN     CMA    MIN II 14.9.
BQ     CMA    B OACT PACCEHHOO CKOEH/IN THE REGION
              OF THE OPEN CLUSTER NGC 2354.
BS     CMA    MIN II 14.5.
CC     CMA    CPEH POBEH ECKA MEHETC?/MEAN BRIGHT-
              NESS VARIES?
CE     CMA    MIN II 13.3. MIN II-MIN I=0.663P.
CH     CMA    MIN II 12.9.
CK     CMA    MIN II 15.4.
CM     CMA    MIN II 13.1.
CO     CMA    CPEH POBEH ECKA, BEPOTHO, MEHETC C
              P-700**D./MEAN BRIGHTNESS PROBABLY VARIES WITH
              P-700**D.
CR     CMA    MIN II 12.4.
CV     CMA    MIN II 13.5. DII=0.09P. MIN II-MIN I=0.358P.
CW     CMA    MIN II 8.94. SB 2.
CX     CMA    MIN II 10.3.
DD     CMA    MIN II 11.8.
DE     CMA    MIN II 13.4.
DS     CMA    VB A (B 15.8M, 10", 130G).
DV     CMA    J.D.2425300-27500: P-CM.TA./SEE TABLE;
              OCE/SINCE J.D.2428000 P-400**D.
EF     CMA    D=0.02P.
EW     CMA    VB (DM<=0.5M, 0.102", 112.1G, 1952.203).
              SB (P=0.261975D). MEHEH ECKA C OPTA-
              HO AO HE CBAH. BEA C OOOKO (BE-
              POTHO, POTEHHA ATMOCEPA OHOO  KOM-
              OHEHTOB  OA OOOKA BOKP CCTEM).
              CEKTPAHE CCEOBAH  4592-4596!.
              /BRIGHTNESS VARIATIONS ARE NOT RELATED TO THE OR-
              BITAL PHASE. SHELL STAR (PROBABLY AN EXTENDED AT-
              MOSPHERE OF ONE OF THE COMPONENTS AND THE COM-
              MON SHELL AROUND THE SYSTEM). SPECTRAL STUDIES
               4592-4596!.
EX     CMA    A CAA B TEEHE 2 HOE (8  9 OKTP
              1962)./WAS FAINT FOR 2 NIGHTS (OCTOBER 8 AND 9,
              1962).
EY     CMA    P VAR, DM VAR  3960!. HA OCHOBHOE KOEAHE
              HAKABATC BTOPHE (P=0.2033D  0.1690D);
              EH PB=2.00D  7243!./THE MAIN WAVE IS SUPER-
              IMPOSED BY SECONDARY ONES (P=0.2033D AND
              0.1690D); BEAT EFFECT, PB=2.00D  7243!.
EZ     CMA    SB. B EHTPE  KOEBO OACT HII S 308. EH
              PACCEHHOO CKOEH COLLINDER 121. AHA O-
              XA MAKCMMA ECKA. CTHK-BEPOTHA
              HETPOHHA BEA. OPMA KPBO ECKA, DM,
              A MAKCMMOB  MHMMOB  CPEH ECK
              MEHTC OT CEOHA K CEOH./IN THE CENTRE OF
              THE RING HII REGION S 308. MEMBER OF THE OPEN
              CLUSTER COLLINDER 121. EPOCH OF MAX LIGHT IS GI-
              VEN. THE COMPANION IS PROBABLY A NEUTRON STAR.
              THE SHAPE OF THE LIGHT CURVE, DM, PHASES OF MA-
              XIMA AND MINIMA AND MEAN LIGHT VARY FROM ONE
              OBSERVATIONAL SEASON TO ANOTHER.
FF     CMA    MIN II 7.6. EMEHT TPET TOHEH. EH
              PACCEHHOO CKOEH CR 132A./ELEMENTS
              SHOULD BE IMPROVED. MEMBER OF THE OPEN CLUSTER
              CR 132A.
FM     CMA    MIN II OT TAKE OK, KAK MIN I  6585!./
              MIN II IS ALMOST AS DEEP AS MIN I  6585!.
FN     CMA    VB (6.3M,  7.5M, 0.561", 115.8G, 1978.15). B TA-
              E AH PEE MEHEH CMMAPHOO ECKA.
              CBAHA C TMAHHOCT V B 95. COACHO  6135!
              EPO CHO OTAETC OT TAHOO./RANGE
              OF COMBINED LIGHT VARIATION IS GIVEN IN THE TABLE.
              ASOCIATED WITH THE NEBULA V B 95. ACCORDING TO
               6135!, THE PERIOD CONSIDERABLY DIFFERS  FROM THE
              TABULATED VALUE.
FQ     CMA    MIN II 9.7.
FR     CMA    ADS 4978 AB (6.2M, 10.4M, 4"23G; C 11.62M, 56").
FS     CMA    POTEHHA AO-EBA OOOKA. MCC
               FE II!,  NI II!,  CR II!,  S II!,  OI!, FE II.
              K-TOK (1.6-20 MU M).  PO AMEPOBC-
              KX H TA P CYG EPEMEHH C XAPAKTEPHM
              BPEMEHEM B HECKOKO ACOB.ECK MEHETC
              HA 0.1M OT HO K HO, O 0.03M B TEEHE HO,
              HOA B KOPPE CO CEKTPAHM MEHE-
              HM  6636!. CCEOBAH CEKTPA  7250,
              FE II. IR EXCESS (1.6-20 MU M). P CYG PROFILES OF
              BALMER LINES VARY IN THE TIME SCALE OF HOURS.
              BRIGHTNESS VARIES FROM NIGHT TO NIGHT BY 0.1M AND
              DURING A NIGHT BY 0.03M, SOMETIMES IN CORRELATI-
              ON WITH SPECTRAL CHANGES  6636!. SPECTRAL STUDI-
              ES  7250, 7251, 7253!.
FT     CMA    VB A (B 12.58M, 36", 97G).
FU     CMA    VB  A (B 14.7M, 14", 230G, 1897; C 11.07M, 40", 225G).
FW     CMA    VR VAR, P=31.9045D  6154!.
FZ     CMA    MIN II 8.44. B OACT HII/IN THE HII REGION
              S 295, B ACCOA/IN THE ASSOCIATION CMA OB 1.
GG     CMA    EH PACCEHHOO CKOEH/MEMBER OF THE OPEN
              CLUSTER CR 132A.
GU     CMA    ADS 5713 AB (7.5M, 8.2M, 0.6", 187G, 1919). SB?
              B OACT HII/IN THE HII REGION S 293.
GY     CMA    COACHO/ ACCORDING TO  8380!, OCTOHHA/DOES
              NOT VARY.
GZ     CMA    SB 2.
HK     CMA    AHA OXA MIN./EPOCH OF MIN IS GIVEN.
HL     CMA    1E 0643.0-1648. SB (P-0.217D); LX/LOPT VAR
              (0.002-1).
BETA   CMA    B 1971-72 ECTBOBAA KOMHA TAHX
              EMEHTOB  (EPO P1)  CEX CCTEM
              EMEHTOB:/IN 1971-72 THE OBSERVATIONS WERE
              DESCRIBED BY THE COMBINATION OF THE TABULATED
              ELEMENTS (PERIOD P1) AND THE FOLLOWING SYSTEMS
              OF ELEMENTS: MAX=2441296.0705+0.251300D*E, (P2);
              MAX=2441296.032+0.23904D*E, (P3); MAX=
              =2441296.065+0.12501D*E, (P1/2); MAX=
              =2441296.124+0.12565D*E, (P2/2). EPO EH:
              /BEAT PERIODS:  49.198D, 5.442D, 4.900D. P1 C 1908
              BEBAETC, P2 MEHAETC./SINCE 1908
              P1 INCREASES, P2 DECREASES. B  3454! HAEHO
              12 EPOOB OEPTOHOB  PEOHAHCHX KOEA-
              H./12 OVERTONE AND RESONANCE PERIODS WERE
              FOUND IN  3454!.
EPSILO N**1   CMA ADS 5176 A (B 14.5M, 25", 147G; C 14.0M, 29", 303G,
              1897).
SIGMA  CMA    ADS 5719 A (14.2M, 11", 153G, 1926).
OMEGA  CMA    SB?
R      CMI    SC 4/10 E.
T      CMI    P VAR. MAX=2422456+324.2D*E (J.D.2416610-
              -22800); MAX=2430896+311.2D*E (J.D.2423090-
              -30900); OCE/SINCE J.D.2430900-CM.TA.
              /SEE TABLE.
U      CMI    HAAETC OP HA BOCXOE BETB, HOA
              PHMA B BTOPHOO MAKCMMA. PA-
              K KPBO ECKA C 1904 O 1970.  7368!.
              /THERE IS A HUMP ON THE ASCENDING BRANCH LOOKING
              SOMETIMES AS A SECONDARY MAXIMUM. THE LIGHT
              CURVE FOR 1904-1970  7368!.
X      CMI    P VAR? DS=3.
RS     CMI    D=0.02P:.
RX     CMI    MIN II 14.6; MIN II-MIN I=0.52P:.
RY     CMI    MIN II 12.0:.
SX     CMI    DI<=0.12P. MIN II 13.6.
SY     CMI    P VAR. MAX=2425234.682+0.565900D*E (J.D.
              2425234-708); OCE/SINCE J.D.2436586-CM.
              TA./SEE TABLE.
TU     CMI    MIN II 15.1.
TW     CMI    MIN II 15.6.
TX     CMI    MIN II 14.7.
UZ     CMI    MIN II 12.1.
XZ     CMI    MIN II 9.88. P VAR?
YY     CMI    MIN II 8.88.
YZ     CMI    MU=0.604", P=221.4G. AHA OXA MIN. P VAR; O-
              OHTEH EH:-0.00003919514D E (E+1)/2.
              HA EPOECKE MEHEH ECKA C AMT-
              O 0.12M (11.26-11.38 V) HAKABATC C-
              HE BCK./EPOCH OF MIN IS GIVEN. P VAR; ADDITI-
              ONAL TERM:-0.00003919514D E (E+1)/2. PERIODICAL
              LIGHT VARIATIONS WITH THE AMPLITUDE 0.12M (11.26-
              -11.38 V) ARE SUPERIMPOSED BY STRONG FLARES.
AG     CMI    P VAR. MIN=2434698.670+1.6645729D*E (J.D.2426350-
              34740)  1727!. OCE/SINCE J.D.2437650-CM.
              TA./SEE TABLE.
AH     CMI    EW?
AK     CMI    MIN II 10.3; MIN II-MIN I=0.55P. P VAR. MIN I=
              =2425352.348+0.56589534D*E (J.D.2424880-
              -35550)  1728!. OCE/SINCE J.D.2435600-CM.
              TA./SEE TABLE.
AL     CMI    B HTEPBAE J.D.2424880-25950 HAEH
              PECTABTC EMEHTAM:/OBSERVATIONS IN
              THE INTERVAL J.D.2424880-25950 ARE REPRESENTED
              BY THE ELEMENTS: MAX=2425243.631+0.55050D*E.
              OCE/SINCE J.D.2436590-CM.TA./SEE TABLE.
AM     CMI    MIN II 10.5.
AN     CMI    D=0.02P:.
AO     CMI    D=0.01P:. MIN II 14.5.
BF     CMI    HA/DEPTH OF MIN II 0.05M:.
RS     CAP    CPEH ECK MEHETC C P=3360D./MEAN
              BRIGHTNESS VARIES WITH P=3360D.
RT     CAP    VB A (B 15M, 26", 227G).
RU     CAP    VB A (B 13.6M, 1.6", 86G).
RV     CAP    <P> VAR: MAX=2424334.6612+0.44775262D*E
              (J.D.2417400-33610)  0323!. OCE/SINCE
              J.D.2433850-CM.TA./SEE TABLE. OPMA KP-
              BO ECKA  EPO MEHTC C EPOOM -
              EKTA AKO =225.5D  6464!. OAMT-
              A KOHEH OT HEHX EMEHTOB OCTA-
              ET +-0.032D./LIGHT CURVE AND PERIOD VARY WITH THE
              BLAZHKO EFFECT PERIOD =225.5D  6464!. SEMI-
              AMPLITUDE  OF DEVIATIONS FROM LINEAR ELEMENTS IS
              +-0.032D. 0.14P<=M-M<=0.25P. (K-B)2=0.05.
RW     CAP    D=0.020P. MIN II 9.9. P VAR. MIN I =2418924.594+
              +3.3923922D*E (J.D.2418920-24000)  6774!;
              MIN I =2424003.014+3.3923457D*E (J.D.2424000-
              -34500)  2389!; OCE/SINCE J.D.2435400-CM.
              TA./SEE TABLE.
RX     CAP    MIN II 12.5.
RY     CAP    VB B (A 7.1M, F0; B 6.6", 90G; C 12.0M, 8.5", 58G).
TV     CAP    <P>=67D  1331!.
TW     CAP    P VAR. P=28.6421871D (J.D.2414000-17600);
              P=28.61700115D (J.D.2417600-24000)  1331!;
              MAX=2426211.90+28.59497D*E (J.D.2421400-
              26200)  2390!; MAX=2435664.8+28.5578D*E
              (J.D.2426210-37500)  2309!; OCE/SINCE J.D.
              2437500-CM.TA./SEE TABLE. 0.14P<=M-M<=0.40P.
               FE/H!=-0.72.
TY     CAP    MIN II 10.6. P VAR.MIN I HEL=2432017.956+
              +1.423466D*E (J.D.2425500-35000); OCE/
              SINCE J.D.2435000-CM.TA./SEE TABLE.
UW     CAP    MIN II 11.5; MIN II-MIN I=0.5P. P VAR? MIN I=
              =2434627.290+1.399118D*E (J.D.2427000-35000);
              OCE/SINCE J.D.243500-CM.TA./SEE TABLE.
YZ     CAP    (K-B)2=0.08.
AD     CAP    BHE ATMEH B-V=+1.00./OUTSIDE ECLIPSES
              B-V=+1.00. P VAR?
AE     CAP    CPEH ECK MEHETC C P=2300D./MEAN
              BRIGHTNESS VARIES WITH P=2300D.
DELTA  CAP    VB A (B 15.8M, 69", 94G; C 12.7M, 119", 302G,
              1911); MU=0.391", P=138.8G. MIN II 2.90. OPMA
              KPBO ECKA/THE LIGHT CURVE SHAPE VAR?  3305!.
EPSILO CAP    VB A (B 9.52M, 68.7", 47G).
R      CAR    VB A (B 12M, 2.1", 138G). H2O, SIO MAEP/MASER.
U      CAR    P VAR. MAX=2429023.80+38.753D*E (J.D.2415000-
              29500); OCE/SINCE J.D.2429500-CM.TA.
              /SEE TABLE.
V      CAR    OPMA KPBO ECKA/THE LIGHT CURVE SHAPE VAR?
X      CAR    MIN II 8.6.
Y      CAR    VB A (B 12.22M, 15"; C 12.96M, 30"). SB (P=400-
              -600D)  5119!. B TAE AH EPO P0 OCHOBHO-
              O KOEAH (A=0.58M). EPO EPBOO OEP-
              TOHA P1=2.55954D  5119! (A=0.28M)./THE FUNDA-
              MENTAL MODE PERIOD P0 IS GIVEN IN THE TABLE.
              (A=0.58M). THE FIRST OVERTONE PERIOD P1=2.55954D
               5119! (A=0.28M). P1:P0=0.7032.
RR     CAR    P VAR. <P>=154D (J.D.2421500-23500); <P>=259D
              (J.D.2426400-30100); <P>=154D (J.D.2430400-
              -33100). S 6.5/1**-.
RT     CAR    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              TR 15.
RY     CAR    K CTHK 14.3M PG./THERE IS A CLOSE COM-
              PANION 14.3M PG. P VAR. MAX=2418475+416D*E
              (J.D.2415140-18500); MAX=2429901+417.3D*E
              (J.D.2423600-32900); OCE/SINCE J.D.2434100-
              -CM.TA./SEE TABLE.
ST     CAR    HA/DEPTH OF MIN II 0.27M.
SW     CAR    HA/DEPTH OF MIN II 0.05M.
SZ     CAR    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              NGC 3114.
TX     CAR    OPMA KPBO ECKA/THE LIGHT CURVE SHAPE VAR?
TZ     CAR    CPEH ECK MEHETC C P=1183D; AMT-
              A KOPOTKOO KA BEKA B MAKCMME OO-
              EPOECKOO KOEAH  MAA B MHMME.
              /MEAN BRIGHTNESS VARIES WITH P=1183D; THE AMP-
              LITUDE OF THE SHORT CYCLE IS LARGE IN MEAN BRIGHT-
              NESS MAXIMUM AND SMALL DURING ITS MINIMUM.
UX     CAR    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              IC 2581.
VV     CAR    B PAOHE OEH EHOO CKOEH N 99  7374!
              (10H 36.0M-58G56', 1950.0), OPEHHOO B T-
              MAHHOCT./IN THE REGION OF THE VERY POOR CLUSTER
              N 99  7374! (10H 36.0M-58G56', 1950.0) EMBEDDED
              IN A NEBULA.
VY     CAR    VB A (B 11.07M; B 9V:, 10", 150G). P VAR. KBA-
              PATH EH:/NONLINEAR TERM:-0.000021D*E**2
              (J.D.2410000-44200). OCEHE HAEH
              MOHO PECTABT TAKE HEHM EMEH-
              TAM:/THE LATEST OBSERVATIONS MAY BE REPRESEN-
              TED ALSO BY LINEAR ELEMENTS: MAX=2444161.16+
              +18.9138D*E (J.D.2441000-44200).  A/H!=0.4.
WZ     CAR    P VAR. MAX=2419981.099+23.000945D*E (J.D.
              2410000-20000)  0025!; MAX=2423984.12+
              +23.0054D*E (J.D.2419800-25500)  0322!; MAX=
              =2434914.86+23.0075D*E+0.000025D*E**2 (J.D.
              2434500-41200)  2309!; OCE/SINCE J.D.2434500-
              -CM.TAKE TA./SEE ALSO TABLE.
XX     CAR    P VAR. MAX=2420769.703+15.723704D*E (J.D.
              2410000-22500)  0025!; P=15.7196D (J.D.
              2423000-30000)  0003!; OCE/SINCE J.D.
              2434500-CM.TA./SEE TABLE; PBEEHHE B
              TAE EMEHT COEPAT  KBAPATH EH:
              /ELEMENTS GIVEN IN THE TABLE CONTAIN A NONLINE-
              AR TERM: -0.0000034D*E**2.
XY     CAR     A/H!=0.1.
XZ     CAR     A/H!=0.2.
YZ     CAR    P VAR. KBAPATH EH:/NONLINEAR TERM:
              +0.0000022D*E**2.  A/H!=-0.1.
AE     CAR    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              NGC 3532.
AF     CAR    P VAR. MAX=2434532+433.7D*E (J.D.2420200-
              -34600); OCE/SINCE J.D.2435000-CM.TA.
              /SEE TABLE.
AG     CAR    EHTPAHA BEA AHETAPHO TMAHHOCT
              P.K.289-0.1 HKOO BOEH, BPOEH-
              HO, O-BMOM, BO BPEM HOBOOOHO
              BCK BE OKOO 1000 ET HAA  7052,
              7113!./CENTRAL STAR OF THE LOW-EXCITATION PLANE-
              TARY NEBULA P.K.289-0.1 EJECTED PROBABLY DURING
              A NOVA-LIKE OUTBURST OF THE STAR ADOUT 1000 YEARS
              AGO  7052, 7113!.
AS     CAR    D=0.025P.
AW     CAR    D=0.015P.
BL     CAR    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              TR 16.
BO     CAR     VB A (B 11.05M V, B8III, 10", 41G). CM./SEE
              RT CAR. HE EH CKOEH./CLUSTER NON-MEMBER.
BP     CAR    P=4.82246D?
BS     CAR    B PAOHE CKOEH/IN THE REGION OF THE CLUS-
              TER IC 2602. MIN II 15.3.
BZ     CAR    BOMOHO MEHEHE CPEHEO ECKA C P=1800D.
              /MEAN BRIGHTNESS POSSIBLY VARIES WITH P=1800D.
CD     CAR    B EHTPE CKOEH/IN THE CENTRE OF THE CLUSTER
              CR 236.
CF     CAR    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              NGC 3496.
CI     CAR    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              NGC 3572. D=0.021P?
CO     CAR    D=0.024P?
CV     CAR    D=0.046P. HA/DEPTH OF MIN II 0.05M.
DE     CAR    D=0.016P?
DH     CAR    VB B (A 15.2M V; B 13", 350G). B-V=+0.90M
              (MIN ECKA/BRIGHTNESS).
DI     CAR    HAP C EEOOOHM MEHEHM EC-
              KA C AMTO 1.7M  EMEHTAM MAX=
              =2438553.70+29.210D*E (J.D.2438465-40300)
               5324! HAATC HATEHE OCAEH
              ECKA  4678!. B MAX B-V=+1.34./BESIDES CEP-
              HEID-LIKE LIGHT VARIATIONS WITH THE AMPLITUDE
              1.7M AND ELEMENTS MAX=2438553.70+29.210D*E
              (J.D.2438465-40300)  5324! LARGE WEAKENINGS OF
              BRIGHTNESS ARE OBSERVED  4678!. AT MAX B-V=
              =+1.34.
DK     CAR    D=0.07P.
DM     CAR    D=0.040P.
DP     CAR    D=0.034P. MIN II 13.1.
DS     CAR    D=0.03P.
DU     CAR    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              IC 2602.
DW     CAR    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              CR 228. MIN II 10.3.
EF     CAR    D=0.04P.
EG     CAR    CM./SEE AE CAR.
EH     CAR    VB A (B 15", 320G).
EK     CAR    CM./SEE AE CAR.
EM     CAR    MIN II 8.9.
EN     CAR    B OACT CKOEH/IN THE REGION OF THE CLUS-
              TER TR 18.
EQ     CAR    D=0.030P. MIN II 13.7.
ER     CAR    CM./SEE AE CAR.
ES     CAR    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              NGC 3572.
EZ     CAR    MIN II 9.8.
FI     CAR    P VAR. MAX=2425446.81+13.4542D*E (J.D.
              2423790-35300)  0046, 2309!. OCE/SINCE
              J.D.2435300-CM.TA./SEE TABLE.
FK     CAR    VB.
FO     CAR    VB A (B 14M, 7", 90G). P VAR. MAX=2434922.531+
              +10.3559D*E (J.D.2423700-35300)  6006!; OCE
              /SINCE J.D.2436000-CM.TA./SEE TABLE.
              B-V: +1.13, +1.43.
FP     CAR    D=0.01P:.
FQ     CAR    CM./SEE EN CAR.
FS     CAR    CM./SEE VV CAR. MIN II 10.9.
FT     CAR    COACHO  2197! CEKTPAH KACC C. BO-
              MOHA OKA B OTOECTBEH./ACCORDING
              TO  2197! SPECTRUM C. MISIDENTIFICATION IS POS-
              SIBLE.
FV     CAR    VB A (B 13M, 10", 135G). P VAR. EMEHT, AH-
              HE B TAE, COEPAT BA OOHTEHX
              EHA:/THERE ARE TWO ADDITIONAL TERMS IN THE
              ELEMENTS GIVEN IN THE TABLE: -0.1065D*10**-7*E**2-
              -0.584D*10**-11*E**3. D=0.02P:. MIN II 13.0.
GG     CAR    MIN II 9.5. AOBO-EBA OOOKA./GAS
              AND DUST ENVELOPE.
GH     CAR    CM./SEE EN CAR.
GK     CAR    B PAOHE CKOEH/IN THE REGION OF THE CLUS-
              TER TR 19. MIN II 13.2.
GL     CAR    CM./SEE ES CAR. MIN II 10.31. CCTEMA C BE-
              HEM H AC;/SYSTEM WITH THE APSIDAL MO-
              TION; E=0.157, OMEGA=99G. EMEHT,   PECTABE-
              H MIN I, AHHE B TAE, COEPAT CHCO-
              AHE EH:/THERE ARE SINUSOIDAL TERMS IN
              THE ELEMENTS FOR MIN I GIVEN IN THE TABLE:
              +0.121D SIN (0.094389G*E)-0.007D SIN (0.188778G*E);
              MIN II=2424263.236+2.4222338D*E-
              -0.121D SIN (0.094389G*E)-0.007D SIN (0.188778G*E).
              DII=0.17P.
GM     CAR    CM./SEE VV CAR. MIN II 9.22.
GN     CAR    MIN II 12.1.
GO     CAR    VB A (B 15", 60G).
GP     CAR    MIN II 12.8.
GQ     CAR    MIN II 13.5.
GR     CAR    MIN II 14.0; MIN II-MIN I=0.316P; DII=0.05P.
GV     CAR    BOMOH EH CKOEH/POSSIBLE MEMBER OF
              THE CLUSTER NGC 3532. MIN II 9.1.
GW     CAR    MIN II 9.9.
GZ     CAR    B TAE PBEEH EMEHT MEHEH EC-
              KA  OCHOBHOO KOEAH C AMTO 0.16M.
              /LIGHT ELEMENTS FOR THE FUNDAMENTAL MODE OSCILLA-
              TION WITH AN AMPLITUDE 0.16M ARE GIVEN IN THE
              TABLE.  EPBOO OEPTOHA C AMTO 0.07M
              /FOR THE FIRST OVERTONE OSCILLATION WITH AN AMPLI-
              TUDE 0.07M MAX=2440742.4+2.93424D*E. OX
              MAKCMMOB  AMT PBEEH COACHO
               5175!./EPOCHS OF MAXIMA AND AMPLITUDES ARE GI-
              VEN ACCORDING TO  5175!.
HH     CAR    VB A (B 13.0M, 5", 260G; C 11.11M, 13", 337G;
              D 12.65M, 15", 7G). D=0.02P. MIN II 10.66. P VAR
                8094!. MIN I HEL=2430860.162+3.2315393D*E
              (J.D.2427590-35260)   5292!. B TAE PBEEH
              BOMOHE TEKE EMEHT./POSSIBLE CURRENT
              ELEMENTS ARE GIVEN IN THE TABLE.
HI     CAR    MIN II 10.8.
HK     CAR    VB A (B 12.5M, 4"). PBEEH PEE MEHE-
              H CMMAPHOO ECKA./RANGE OF COMBINED
              BRIGHTNESS VARIATION IS GIVEN.
HL     CAR    D=0.03P:.
HN     CAR    MIN II 12.5.
HP     CAR    VB A (B 9.1M, 0.4", 178G). MIN II 9.3. EMEHT
              TPET TOHEH  8083!./ELEMENTS SHOULD BE
              CORRECTED  8083!.
HQ     CAR    B-V: +0.63, +1.04.
HR     CAR    OCAHE CEKTPA/SPECTRUM DESCRIPTION  1914,
              6466!.
HT     CAR    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              IC 2581. MIN II 14.0.
HV     CAR    D=0.026P. MIN II 14.2.
HW     CAR    AHA OXA MIN./EPOCH OF MIN IS GIVEN.
HX     CAR    MIN II 14.5.
IK     CAR    CM./SEE DU CAR.
IL     CAR    MIN II 14.4.
IN     CAR    BOMOHO, EPO CEET BOT./IT IS POSSIB-
              LE THAT THE PERIOD MUST BE DOUBLED.
IQ     CAR    CM./SEE AE CAR.
IR     CAR    CM./SEE AE CAR. MIN II 12.6.
IS     CAR    MIN II 14.0.
IU     CAR    (K-B)2=0.02.
IW     CAR    CPEH ECK MEHETC C EPOOM OKOO 1500D,
              AMTA OCHOBHOO KOEAH-OT 1.3M O 0.3M.
              /MEAN BRIGHTNESS VARIES WITH THE PERIOD CLOSE TO
              1500D, THE AMPLITUDE OF MAIN OSCILLATIONS-FROM
              1.3M TO 0.3M.
IX     CAR    B EHTPE PKO TMAHHOCT AMETPOM 2.4'./IN
              THE CENTRE OF A BRIGHT NEBULA WITH THE DIAMETER 2.4'.
KQ     CAR    MIN II 10.3.
KU     CAR    MIN II 11.6.
MP     CAR    VB A (B 16M, 180G).
MZ     CAR    .-B. KOMOHEHT TECHO AP./SF COMPONENT OF
              A CLOSE PAIR.
OO     CAR    MIN II 14.7.
OV     CAR    MIN II 13.5.
OY     CAR    EMEHT ATMEH:/ECLIPSE ELEMENTS:
              MIN I HEL=2443993.553241+0.0631209247D*E
               5185!; D=0.050P, D=0.044P. OP HA KPBO
              ECKA HA AE 0.75P./THE HUMP ON THE LIGHT
              CURVE IS OBSERVED AT THE PHASE OF 0.75P. -
              HA MIN I MEHETC B PEEAX 1.48M-2.47M.
              /DEPTH OF MIN I VARIES BETWEEN 1.48M AND 2.47M.
PT     CAR    MIN II 13.0:.
PX     CAR    MIN II 10.10.
QR     CAR    MIN II 10.4.
QS     CAR    MIN II 9.3.
QU     CAR    HDE 310376 (HA 112, 173). KTA ECKA
              HAOMHAT V 818 SCO, MEHEH HA 0.2M A
              90C. EPOHOCT HE OHAPEHA. B CEKTPE
              MCC HE II 4686, CIV-NIII 4630-4650, HO-
              A CA BOOPOH CEKTP OOEH, CO-
              OTBETCTB KACC A  B  5643!./FLICKE-
              RING RESEMBLES V818 SCO. VARIATIONS BY 0.2M IN 90S
              WERE OBSERVED. NO PERIODICITY WAS FOUND. EMIS-
              SION LINES HE II 4686, CIV-NIII 4630-4650 AND
              SOMETIMES WEAK HYDROGEN ABSOPTIONS (CORRESPON-
              DING TO A OR B TYPE) ARE NOTICEABLE IN THE SPE-
              CTRUM  5643!.
QX     CAR    MIN II 7.02.
QY     CAR    B PACCEHHOM CKOEH/IN THE OPEN CLUSTER
              NO.90  7374!.
QZ     CAR    B TMAHHOCT ETA K, BOMOH EH CKO-
              EH COLLINDER 228./IN THE ETA CARINA NEBULA,
              POSSIBLE MEMBER OF THE CLUSTER COLLINDER 228.
              MIN II 6.43. BE SB1-CCTEM (A  B),
              ATMEHHA-B/TWO SB 1 SYSTEMS (A AND B),
              B IS ECLIPSING (A: SB 1, P=20.73D, O9.5 I,
              DM=0.6M). AH CMMAPH ECK./COMBINED
              BRIGHTNESS IS GIVEN.
V 341  CAR    B OTPAATEHO TMAHHOCT EPEMEHHO P-
              KOCT IC 2220. B PAOHE PACCEHHOO CKOE-
              H NGC 2516. K TOK./IN THE VARIABLE
              REFLECTING NEBULA IC 2220. IN THE REGION OF THE
              OPEN CLUSTER NGC 2516. IR EXCESS.
V 343  CAR    VB. SB (P=133.92D).
V 347  CAR    OK/DEEP MIN II.
V 348  CAR    B PACCEHHOM CKOEH/IN THE OPEN CLUSTER
              IC 2581. MIN II 8.9.
V 354  CAR    OEH KPACHA./VERY RED.
V 356  CAR    EH CKOEH/MEMBER OF THE CLUSTER
              NGC 2516.
V 357  CAR    SB (P=6.74483D  4627!).
V 361  CAR    B OACT CKOEH/IN THE REGION OF THE CLUS-
              TER NGC 3293.
V 365  CAR    CM./SEE AE CAR.
V 367  CAR    MIN II 7.54.
V 373  CAR    CM./SEE V 356 CAR.
V 374  CAR    CM./SEE V 356 CAR.
V 375  CAR    P=0.264D /OR 0.359D.
V 376  CAR    VB A (B 6.83M, B 9.5V, 41", 75G).
V 378- V 381  CAR B PACCEHHOM CKOEH/IN THE OPEN
              CLUSTER NGC 3293.
V 382  CAR    B OACT CKOEH/IN THE REGION OF THE CLUS-
              TER NGC 3532.
V 385  CAR    HA/DEPTH OF MIN II 0.04M. OKPEHA
              KOEBO TMAHHOCT/SURROUNDED BY A RING
              NEBULA RCW 58.
ETA    CAR    B MCCOHHO TMAHHOCT NGC 3372 B PAOHE
              CKOEH TR 16. OEH MACCBHA MOOA
              BEA, OKPEHHA PACPEC AOBO--
              EBO OOOKO AMETPOM OT 2" HA BOHE 2 MU
              O 6.5" HA 12.2 MU. MAKCMMA ECKA OCTA
              B 1843. C 1880.ECK MEHETC B PEEAX
              5.9 -7.9 V. B HTEPBAE J.D.2434000-41000
              HAAAC KHOCT MEHEH ECKA:
              MAX=2434037+1110D*E. B CEKTPE PKE H
              H, HEI, FE II,   FE II!  P. OCAHE CEKTPA
               5251, 7279!. CTOHK MKOO PEHTEHOBCKOO
              EH EPEMEHHO HTEHCBHOCT./IN THE
              EMISSION NEBULA NGC 3372 IN THE REGION OF THE
              CLUSTER TR 16. A VERY MASSIVE YOUNG STAR SURRO-
              UNDED BY AN EXPANDING GAS AND DUST SHELL WITH
              THE DIAMETER 2" AT 2MU AND 6.5" AT 12.2MU. MAXI-
              MUM BRIGHTNESS WAS OBSERVED IN 1843. SINCE
              1880 VARIES IN THE RANGE 5.9-7.9 V. IN THE INTER-
              VAL J.D.2434000-41000 MAX=2434037+1110D*E.
              THERE ARE EMISSION LINES OF H, HEI, FEII,  FEII!,
              ETC. IN THE SPECTRUM. DESCRIPTION OF THE SPECTRUM
               5251, 7279!. SOFT X-RAY SOURCE OF VARIABLE INTEN-
              SITY.
HI     CAR    CTOHK MKOO PEHTEHOBCKOO EH.
              /SOFT X-RAY SOURCE.
R      CAS    VB A (B 14.5M, 14", 273G). SIO, OH MAEP/MASER;
              HOA H2O MCC/SOMETIMES H2O EMISSION.
T      CAS    SIO MAEP/MASER. B HPAKPACHO OACT
              CEKTPA-OOC ZRO./ZRO BANDS IN THE INFRA-
              RED SPECTRAL REGION.
U      CAS    S 4.5/4E.
W      CAS    SC 5/9E.
X      CAS    P VAR: MAX=2426650+432.32D*E (J.D.2416750-
              -27060); MAX=2432870+413.6D*E (J.D.2427060-
              -32870); MAX=2437948+423.0D*E (J.D.2432870-
              -39210). B TAE AH TEKE EMEHT.
              /CURRENT ELEMENTS ARE GIVEN IN THE TABLE.
Y      CAS    OH, H2O MCC/EMISSION; SIO MAEP/MASER.
Z      CAS    SIO MAEP/MASER.
RS     CAS    P VAR. MAX=2416942.16+6.29552D*E (J.D.2412650-
              34900)  3317!. OCE/SINCE J.D.2434900-CM. TA.
              /SEE TABLE.
RV     CAS    B CEKTPE-PHAK KACCA SE  3383!./THERE
              ARE SIGNS OF SE TYPE IN THE SPECTRUM  3383!.
RW     CAS    P VAR. MAX=2421354.22+14.8004D*E (J.D.2417000-
              -30000). OCE/SINCE J.D.2430000-CM. TA.
              /SEE TABLE.  A/H!=0.3.
RX     CAS    HKAHA CTPO BOOHPA ATMEH-
              HA CCTEMA./UNIGUE RAPIDLY EVOLVING ECLIPSING
              SYSTEM. MIN II 9.49; MIN II-MIN I=0.5070P. P VAR.
              KBAPATH EH:/NONLINEAR TERM:
              +1.017D*10**-5*E**2. HAEH MOHO PECTABT
              TAKE TPEM CCTEMAM EMEHTOB:/OBSERVATI-
              ONS MAY BE REPRESENTED ALSO BY THREE SYSTEMS OF
              ELEMENTS: MIN I=2416250.889+32.31481D*E
              (0<=E<=286, J.D.2416250-25482); MIN I=
              =2416248.835+32.32145D*E (331<=E<=554, J.D.
              2426940-34155); MIN I=2416244.990+
              +32.32765D*E (734<=E<=876, J.D.2439970-44570).
              ECK CCTEM BHE ATMEH EPOECK ME-
              HETC B PEEAX 8.6M-9.0M C EMEHTAM:
              /BRIGHTNESS OF THE SYSTEM OUT OF ECLIPSES PERIODI-
              CALLY VARIES WITHIN 8.6M-9.0M WITH ELEMENTS:
              MAX=2416198+516.06D*E  5036!. MAX-MIN=
              =233D=0.45P  0881!. CHE MCC/STRONG
              EMISSIONS OF H, NV, CIV, SIIV, FEIII. BOMO-
              HO HAE MOHOO AOBOO OTOKA  BEH
              AKKPE./POWERFUL GASEOUS STREAM AND ACCRETION
              PHENOMENA ARE POSSIBLE.
RY     CAS     A/H!=0.0.
RZ     CAS    MIN II 6.26. OPMA KPBO ECKA/THE LIGHT CUR-
              VE SHAPE VAR; D VAR (0.000P<=D<=0.009P). P VAR,
              MEHEH HEPABHE. CPEHE EMEHT
              O BAHM  OTOPAECKM HAEH-
              M ECKA:/P VAR, VARIATIONS ARE IRREGULAR. MEAN
              ELEMENTS BASED ON VISUAL AND PHOTOGRAPHIC OBSER-
              VATIONS: MIN I=2416886.8806+1.195253065D*E
              (J.D.2416800-26700)  8820!, MIN I=2432820.7853+
              +1.1952517D*E (J.D.2426700-34000)  0938!. O
              OTOEKTPECKM HAEHM:/FROM PHOTO-
              ELECTRIC OBSERVATIONS: MIN I=2432115.5827+
              +1.1952472D*E (J.D.2429870-30400); MIN I=
              =2432085.7011+1.195259D*E (J.D.2432000-
              -32460); MIN I=2434349.5130+1.1952525D*E
              (J.D.2432450-34420); MIN I=2434703.3035+
              +1.195238D*E (J.D.2434420-34705); MIN I=
              =2435934.4087+1.1952499*E (J.D.2434705-
              -35950); MIN I=2438829.2818+1.195243D*E
              (J.D.2436800-39100); MIN I=2440182.3089+
              +1.195259D*E (J.D.2439380-40200); MIN I=
              =2441333.3257+1.195244D*E (J.D.2440500-
              -41350); MIN I=2442327.7798+1.1952521D*E
              (J.D.2441550-42350); OCE/SINCE J.D.2442850-
              -CM. TA./SEE TABLE.
SU     CAS     A/H!=-0.1.
SV     CAS    P VAR. MAX=2421839+279.3D*E (J.D.2417600-
              -21900); MAX=2430450+281.7D*E (J.D.2422500-
              -31900); OCE/SINCE J.D.2432600-CM. TA.
              /SEE TABLE.
SX     CAS    VB A (B 11.5M, 19", 250G, 1966). MIN II 9.32.
              OPMA KPBO ECKA/THE LIGHT CURVE SHAPE VAR.
              DII=0.171P:, DI=0.036P, DII=0.050P. P VAR.
              MIN I=2433963.267+36.56727D*E (J.D.2418000-
              -37000); OCE/SINCE J.D.2438700-CM. TA.
              /SEE TABLE. CHE MCC/STRONG EMISSIONS
              OF H, NV, CIV, SIIV, FEIII. AOBE OTOK 
              BEH AKKPE./GASEOUS STREAMS AND ACCRE-
              TION PHENOMENA.
SY     CAS    VB? P VAR. MAX=2417911.547+4.070969D*E (J.D.
              2417000-34000); OCE/SINCE J.D.2434000-CM.
              TA./SEE TABLE.
SZ     CAS    P VAR. MAX=2421261.66+13.6009D*E (J.D.2416700-
              -21260); MAX=2426650.20+13.6072D*E (J.D.
              2421260-27170)  8821!; MAX=2429727.240+
              +13.61744D*E (J.D.2427170-33050); MAX=
              =2436810.92+13.62655D*E (J.D.2433050-38720);
              OCE/SINCE J.D.2438720-CM. TA./SEE TABLE.
               A/H!=-0.6.
TU     CAS    AMTA KOEAH C OCHOBHM EPOOM P0,
              AHHM B TAE, PABHA 0.69M. CPEH AM-
              TA KOEAH C EPOOM EPBOO OEPTOHA
              P1=1.51830D A 67 ET MEHAC OT 0.4M O
              0.25M  5078!./FUNDAMENTAL MODE PERIOD P0 IS
              GIVEN IN THE TABLE; THE CORRESPONDING AMPLITUDE
              IS 0.69M. FIRST-OVERTONE PERIOD P1=1.51830D; THE
              CORRESPONDING MEAN AMPLITUDE DECREASED FROM
              0.4M TO 0.25M DURING 67 YEARS  5078!. P1/P0=0.71.
              M-M VAR (0.17P<=M-M<=0.35P).
TV     CAS    D=0.01P. MIN II 7.34. OPMA KPBO ECKA/THE
              LIGHT CURVE SHAPE VAR. EPO TX MEHEH
              /PERIOD OF THESE VARIATIONS-600D  8822!. P VAR.
              CPEHE EMEHT O BAHM  OTOPA-
              ECKM HAEHM ECKA:/MEAN ELEMENTS
              BASED ON VISUAL AND PHOTOGRAPHIC OBSERVATIONS:
              MIN I=2432827.7665+1.81260983D*E (J.D.2415650-
              -32800)  1926!. O OTOEKTPECKM HA-
              EHM/FROM PHOTOELECTRIC OBSERVATIONS MIN I=
              =2432827.7665+1.8126142D*E (J.D.2432800-
              -36490); MIN I=2436483.8091+1.81255D*E (J.D.
              2436480-36980); MIN I=2438472.2386+1.81263D*E
              (J.D.2437000-38500); MIN I=2438829.3230+
              +1.8126048D*E (J.D.2438470-41750); OCE/SIN-
              CE J.D.2441750-CM. TA./SEE TABLE.
TW     CAS    MIN II 8.40.
TX     CAS    MIN II 9.6.
TY     CAS    P VAR. MAX=2419260+545.0D*E (J.D.2419200-25300);
              MAX=2428965+623.8D*E (J.D.2427000-41500); OC-
              E/SINCE J.D.2441500-CM. TA./SEE TABLE.
UU     CAS    MIN II 10.5.
UZ     CAS     A/H!=-0.3.
VV     CAS    P VAR. MAX=2422514.16+6.207510D*E (J.D.
              2417000-32500); OCE/SINCE J.D.2432500-CM.
              TA./SEE TABLE.  A/H!=-0.2.
VW     CAS     A/H!=0.0.
WY     CAS    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              NGC 7789. B MHMME ECKA BEH CEKTP
              BE KACCA G  3502!. BOMOHO, CECTBO-
              BAHE ECKOO CTHKA./THE SPECTRUM OF
              THE G TYPE STAR IS SEEN IN MINIMUM LIGHT  3502!. THE
              EXISTENCE OF A PHYSICAL COMPANION IS POSSIBLE. S 6/6-E.
WZ     CAS    VB A (OTECK CTHK/OPTICAL COMPANION
              B 8.7M, 58", 89G). SC 7/10E. HOA MEHEH ECKA
              POCXOT C BOEHHM EPOOM./LIGHT VARIATIONS
              ARE SOMETIMES TAKING PLACE WITH DOUBLED PERIOD.
XX     CAS    MIN II 10.2.
YZ     CAS    VB A (B 11.23M, 35", 160G). D=0.045P. MIN II 5.78.
ZZ     CAS    MIN II 10.9.
AB     CAS    EA/SD. MIN II 10.28. P VAR. MIN I=2430755.678+
              +1.366863D*E (J.D.2425400-33150); MIN I=
              =2433616.532+1.366876D*E (J.D.2433150-37000);
              MIN I=2440475.5216+1.3668783D*E (J.D.2437000-
              -41600); OCE/SINCE J.D.2441600-CM. TA.
              /SEE TABLE. KOMOHEHT A3-EPEMEHHA TA
              DSCT C EMEHTAM:/THE A3 COMPONENT IS A
              DSCT TYPE VARIABLE WITH THE ELEMENTS: MAX HEL=
              =2444912.1759+0.0582874D*E  8825!; AMTA
              CA DV/AMPLITUDE OF PULSATIONS DV VAR
              (0.03M<=DV<=0.09M).
AE     CAS    MIN II 12.8.
AH     CAS    MIN II 13.3.
AL     CAS    MIN II 13.6.
AO     CAS    MIN II 6.24. OPMA KPBO ECKA/THE LIGHT CUR-
              VE SHAPE VAR. P VAR?
AQ     CAS    MIN II 10.4.
AR     CAS    VB A (B 9.3M, 1.0", 336G; C 8.2M, 75", 269G;
              D 9.8M, 76", 268G; E 11.28M, 43", 115G; F 11.06M, 69",
              338G; G 11.11M, 67", 348G). MIN II 4.86; MIN II-MIN I=
              =0.614P; DII=0.076P; DII=0.037P.
AS     CAS    VB A (B 15.5M, 3", 45G). AMTA KOEAH
              C OCHOBHM EPOOM P0, AHHM B TAE,
              PABHA 0.59M. AMTA KOEAH C EPOOM
              P1=2.2909D PABHA 0.13M./FUNDAMENTAL MODE PE-
              RIOD P0 IS GIVEN IN THE TABLE; THE CORRESPONDING
              AMPLITUDE IS 0.59M. FIRST-OVERTONE PERIOD P1=
              =2.2909D; AMPLITUDE OF OSCILLATIONS WITH THIS PE-
              RIOD IS 0.13M. P1/P0=0.76.
AX     CAS    MIN II 12.9.
AZ     CAS    B-V:+1.78, +2.20. D=110D, D=88D=0.026P.
BD     CAS    B-V:+1.50, +1.61. P VAR. MAX=2429124.84+
              +3.65129D*E (J.D.2415000-29130)  0915!; OC-
              E/SINCE J.D.2429130-CM. TA./SEE TABLE.
BE     CAS    VB A (B G, 25", 260G).
BH     CAS    COACHO  0453!, HA MECTE BH CAS  B EE OKPECT-
              HOCTX HET EPEMEHHX BE./ACCORDING TO
               0453! THERE ARE NO VARIABLE STARS ON THE PLACE OF
              BH CAS AND IN ITS SURROUNDINGS.
BM     CAS    MIN II 8.98. OPMA KPBO ECKA MEHETC.
              /SHAPE OF THE LIGHT CURVE VARIES. P VAR. EMEHT
              COEPAT CHCOAH EH:/THERE IS A PERIO-
              DIC TERM IN THE ELEMENTS:+2.6D SIN (7G. 11*E+104G).
              COACHO  0939! HA KPBO ECKA HAATC
              EEOOOHE KOEAH C P=27D./ACCORDING
              TO  0939! ON THE LIGHT CURVE CEPHEID-LIKE VARIATI-
              ONS ARE OBSERVED WITH P=27D.
BN     CAS    MIN II 13.4.
BS     CAS    MIN II 12.6.
BU     CAS    D=0.02P.
BY     CAS    B OACT CKOEH/IN THE REGION OF THE CLUSTER
              NGC 663. P VAR. MAX=2416871.91+3.2218D*E (J.D.
              2416800-24860)  0921!; MAX=2431929.60+
              +3.221297D*E (J.D.2426900-34300); MAX=
              =2438399.629+3.222588D*E (J.D.2436200-39400);
              OCE/SINCE J.D.2439400-CM. TA./SEE TABLE.
BZ     CAS    MIN II 11.5.
CC     CAS    MIN II 7.26. OPMA KPBO ECKA/THE LIGHT CUR-
              VE SHAPE VAR? P VAR?
CEA    CAS    BOMOH EH CKOEH NGC 7790./POSSIBLE
              MEMBER OF THE CLUSTER NGC 7790. VB A (B=
              =CEB CAS, 2.4", 265G).
CEB    CAS    VB B (A=CEA CAS). CM./SEE CEA CAS.
              OF THE CLUSTER NGC 7790.  A/H!=0.1.
CG     CAS    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              NGC 7790.
CH     CAS     A/H!=-0.5.
CQ     CAS    HA MEEHHE KOEAH HAKABATC OEE
              CTPE C KAM OT 110D O 250D./THE SLOW
              OSCILLATIONS ARE SUPERIMPOSED BY MORE RAPID ONES
              WITH CYCLES FROM 110D TO 250D.
CR     CAS    MIN II 13.3.
CS     CAS     A/H!=-0.4.
CV     CAS    OX, AHHE B  0922!, HE PECTABTC P-
              BEEHHM EMEHTAM./EPOCHS GIVEN IN  0922!
              ARE NOT REPRESENTED BY THE ELEMENTS GIVEN IN THE
              TABLE. P VAR?
CW     CAS    MIN II 11.47. OPMA KPBO ECKA  H
              MHMMOB MEHTC./SHAPE OF THE LIGHT CURVE
              AND DEPTHS OF MINIMA VARY. P VAR. MIN I=
              =2435745.6163+0.31886497D*E (J.D.2432400-
              -41000)  3332!; OCE/SINCE J.D.2441000-CM.
              TA./SEE TABLE.
CY     CAS     A/H!=-0.7.
DD     CAS    P VAR. MAX=2415612.45+9.807272D*E (J.D.
              2415600-18600); OCE/SINCE J.D.2418600-CM.
              TA./SEE TABLE. BOMOHO, EH BOHO CCTE-
              M C PORB=8500D+-1000D./THE STAR MAY BE A
              MEMBER OF A BINARY SYSTEM WITH PORB=8500D+-
              +-1000D.
DF     CAS    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              NGC 1027.
DI     CAS    P VAR. MAX=2432068+371.7D*E (J.D.2417200-
              32100); OCE/SINCE J.D.2432100-CM. TA.
              /SEE TABLE.
DL     CAS    EH CKOEH/MEMBER OF THE CLUSTER NGC 129.
               A/H!=0.0.
DN     CAS    MIN II 10.13.
DO     CAS    MIN II 8.61; DI=0.08P.
DP     CAS    MIN II 13.6.
DZ     CAS    MIN II 12.0.
EG     CAS    MIN II 13.1.
EK     CAS    HA/DEPTH OF MIN II 0.05M.
EM     CAS    P VAR. MAX=2433132+283D*E (J.D.2427700-
              33150); OCE/SINCE J.D.2433150-CM. TA.
              /SEE TABLE. AMTA CHO MEHETC./AM-
              PLITUDE STRONGLY VARIES.
EN     CAS    MIN II 12.4. P VAR.
EP     CAS    MIN II 11.4.
EQ     CAS    MIN II 12.7. P VAR. MIN I=2432150.04+58.26D*E
              (J.D.2432200-34060)  3336!; OCE/SINCE J.D.
              2436100-CM. TA./SEE TABLE.
EY     CAS    MIN II 14.5.
GG     CAS    D=0.013P. MIN II 9.99. P VAR? MIN I=2430188.468+
              +3.758738D*E (J.D.2424800-39500)  0936!; OC-
              E/SINCE J.D.2439500-CM. TA./SEE TABLE.
GK     CAS    HA/DEPTH OF MIN II 0.05M.
GT     CAS    D=0.02P.
GU     CAS    MIN II 11.3. P VAR. MIN I=2428749.423+
              +3.093329D*E (J.D.2417470-35480)  0941!;
              MIN I=2437367.375+3.09325D*E (J.D.2435480-
              -38750)  0001!; OCE/SINCE J.D.2438750-CM.
              TA./SEE TABLE.
GZ     CAS    CPEH BEHA MEHETC C EPOOM 800D.
              /MEAN MAGNITUDE VARIES WITH P=800D. MAX=
              =2428000+800D*E  0911!.
HH     CAS    AHA OXA MIN. BOMOEH T RV  0911!.
              /EPOCH OF MIN IS GIVEN. RV TYPE IS POSSIBLE
               0911!.
HN     CAS    D=0.038P.
HS     CAS    VB A (B 12M, 27", 15G).
HT     CAS    MIN HEL=2443727.93722+0.073647217D*E;
              D=0.13P. ME BCKAM HA ATMEH
              -2.4M V./DEPTH OF ECLIPSES BETWEEN OUTBURSTS
              IS-2.4M V. HEOE KBAEPOECKE KO-
              EAH ECKA C P=100S./SMALL GUASI-PERIODIC
              LIGHT OSCILLATIONS WITH P=100S. OCAHE CEKT-
              PA/SPECTRUM DESCRIPTION  6163!.
HU     CAS    P VAR. MAX=2417525.075+0.41159875D*E (J.D.
              2411600-28000); OCE/SINCE J.D.2428000-
              -CM. TA./SEE TABLE.
IL     CAS    HA/DEPTH OF MIN II 0.05M.
IR     CAS    MIN II 11.5. P VAR. MIN I=2428750.2914+
              +0.68069178D*E (J.D.2417500-38400)  0098!;
              OCE/SINCE J.D.2438400-CM. TA./SEE TABLE.
IS     CAS    MIN II 12.2. P VAR. MIN I=2428776.262+
              +1.8415172D*E (J.D.2417400-29500)  0098!;
              OCE/SINCE J.D.2428000-CM. TA./SEE TABLE.
IT     CAS    MIN II 11.8; MIN II-MIN I=0.553P; DII=0.042P.
              BOMOHO BEHE H AC./APSIDAL MO-
              TION IS POSSIBLE.
IV     CAS    MIN II 11.3. P VAR. MIN I=2428991.302+
              +0.9985232D*E (J.D.2416700-29000)  0098!;
              MIN I=2431438.648+0.9985056D*E (J.D.2429000-
              -37700)  2263!; OCE/SINCE J.D.2440000-CM.
              TA./SEE TABLE.
IW     CAS    S 4+/6 E.
IX     CAS    P VAR. MAX=2428749.39+9.15035D*E (J.D.2414700-
              -29500)  0098!; MAX=2428749.90+9.1363D*E
              (J.D.2428700-34350)  0944!; MAX=2437195.642+
              +9.14783D*E (J.D.2434350-39100)  5462!; OCE
              /SINCE J.D.2442000-CM. TA./SEE TABLE.
               A/H!=-0.4.
KL     CAS    MIN II 12.3.
KO     CAS    P VAR. MAX=2425590+305.6D*E (J.D.2416700-
              -26000); OCE/SINCE J.D.2426000-CM. TA.
              /SEE TABLE.
KR     CAS    MIN II 9.9.
LR     CAS    MIN II 10.9.
LU     CAS    MIN II 14.3?
LW     CAS    B BEPHE MAEHKO (8") PKO KOMETOOPA-
              HO TMAHHOCT B PAOHE IC 1848. B HTEPBAE
              J.D.2433900-34800 HAAAC HOBOOOHA
              BCKA./IN THE APEX OF A SMALL (8") BRIGHT CO-
              METARY NEBULA IN THE REGION OF IC 1848. NOVALI-
              KE OUTBURST WAS OBSERVED IN THE INTERVAL J.D.
              2433900-34800. HPAKPACHOE  PAOE-
              HE./INFRARED AND RADIOEMISSION.
LX     CAS    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              COLLINDER 33. MIN II 15.3; MIN II-MIN I=0.47P;
              DI=0.10P.
LY     CAS    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              COLLINDER 33. MIN II 15.2.
MM     CAS    D=0.08P: MIN II 12.4.
MN     CAS    MIN II 10.57.
MO     CAS    B TMAHHOCT/IN THE NEBULA NGC 7635.
              10.2-13.1 I.
MP     CAS    B TMAHHOCT/IN THE NEBULA NGC 7635.
              10.4-13.5 I.
MR     CAS    MIN II 15.5.
MS     CAS    MIN II 13.2.
MT     CAS    D=0.04P. MIN II 14.02.
MU     CAS    MIN II 10.8.
MV     CAS    MIN II 14.0.
MY     CAS    MIN II 15.2. P VAR. EMEHT, AHHE B TA-
              E, PECTABT HAEH OCE J.D.
              2438500./ELEMENTS GIVEN IN THE TABLE ARE VALID
              SINCE J.D.2438500.
NN     CAS    MIN II 14.0.
NT     CAS    MIN II 14.4.
NU     CAS    MIN II 13.4.
NV     CAS    D=0.03P.
OP     CAS    P VAR. MAX=2429109.726+5.510019D*E (J.D.
              2427950-34670)  0176!; OCE/SINCE J.D.
              2437000-CM. TA./SEE TABLE.
OR     CAS    MIN II 11.8. P VAR. MIN I=2429249.424+
              +1.2457026D*E (J.D.2413800-34800)  0176!;
              OCE/SINCE J.D.2432000-CM. TA./SEE TABLE.
OX     CAS    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              NGC 381. D=0.016P. MIN II 10.30; MIN II-MIN I=
              =0.512P. BEHE H AC  4524!./APSIDAL
              MOTION  4524!.
PR     CAS    P=171D?
PV     CAS    MIN II 10.36; MIN II-MIN I=0.480P. HA M-
              HMMOB, BOMOHO, MEHETC./DEPTH OF MINI-
              MA PROBABLY VARIES. P VAR. MIN I=2428796.8142+
              +1.75047346D*E (J.D.2415700-40000)  5302!; OC-
              E/SINCE J.D.2440000-CM. TA./SEE TABLE.
              BEHE H AC  6253!:/APSIDAL MOTION
               6253!: MIN II=2428797.6894+1.75047346D*E-
              -0.040D SIN 0.0075G, (E-3000).
PX     CAS    MIN II 15.0.
PY     CAS    AHA OXA MIN ECKA. O OPME KPBO EC-
              KA OOHA RV TAU  3348!./EPOCH OF MIN BRIGH-
              NESS IS GIVEN. SIMILAR TO RV TAU BY LIGHT CURVE
              SHAPE  3348!.
PZ     CAS    VB A (B 12.8M, WN 8:, 15", 100G). OH, H2O MC-
              C/EMISSION.
QQ     CAS    MIN II 10.8. P VAR. MIN I=2434330.169+2.142030D*E
              (J.D.2415700-30000)  2530!; OCE/SINCE J.D.
              2430000-CM. TA./SEE TABLE.
QX     CAS    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              NGC 7790. VB A (B 13.1M, 3"). MIN II 10.50;
              MIN II-MIN I=0.37P; DII=0.047P; DII=0.018P.
V 336  CAS    MIN II 13.6.
V 341  CAS    D=0.031P.
V 344  CAS    MIN II 13.4.
V 345  CAS    MIN II 13.6.
V 357  CAS    MIN II 13.6.
V 359  CAS    MIN II 12.0.
V 360  CAS    MIN II 12.3.
V 361  CAS    D=0.051P.
V 363  CAS    DS=1.
V 364  CAS    MIN II 11.9.
V 365  CAS    S 6/3-.
V 366  CAS    MIN II 12.7. P VAR. MIN I=2435075.461+
              0.7292714P*E (J.D.2414600-35400)  2305!;
              OCE/SINCE J.D.2434650-CM. TA./SEE
              TABLE.
V 373  CAS    HKAHA TECHA BOHA. PORB=
              =13.4192D  4627!. PBEEHA OXA MIN I
              ECKA, KA K MOMEHT OHOO  COE-
              HEH. MIN II-MIN I=0.58P. MAKCMM OEH
              OCTPE. MAX-MIN II=0.25P. HE CKEHO,
              TO BEA BETC ATMEHHO C EC-
              KM MEHEHM ECKA KOMOHEHTOB, HO
              ATMEH, EC OH CECTT, OCOB-
              BAT  OEH HEO ACT HAA-
              EMX MEHEH ECKA. PEE MEHE-
              H ECKA PBEEH O AHHM  2651!.
              OHO AMTA KA K 0.1M./A UNIGUE
              CLOSE BINARY. PORB=13.4192D  4627!. EPOCH
              OF MIN I IS GIVEN CLOSE TO THE EPOCH OF ONE
              OF CONJUNCTIONS. MIN II-MIN I=0.58P. MAXIMA
              ARE VERY SHARP. MAX-MIN II=0.25P. IT IS NOT
              EXCLUDED THAT THE STAR IS AN ECLIPSING ONE
              WITH PHYSICAL VARIABILITY OF COMPONENTS, BUT
              ECLIPSES, IF THEY EXIST, CAUSE ONLY A VERY
              SMALL PART OF THE OBSERVED LIGHT VARIATIONS.
              RANGE OF LIGHT VARIATIONS IS GIVEN ACCORDING
              TO  2651!. AS A RULE THE AMPLITUDE IS CLOSE TO
              0.1M.
V 374  CAS    MIN II 12.1.
V 375  CAS    MIN II 10.6.
V 377  CAS    VB (A 8.5M; B 9.4M, 2.1", 185G, 1962). HEBE-
              CTHO, KAKO  KOMOHEHTOB MEHETC./IT IS
              NOT KNOWN WHICH COMPONENT VARIES. COACHO
               4005! AMTA MEHEH CMMAPHOO
              ECKA 0.26M./ACCORDING TO  4005! THE RANGE
              OF COMBINED BRIGHTNESS VARIATIONS IS 0.26M.
              COACHO/ACCORDING TO  7051!, CONST.
V 380  CAS    D=0.08P.
V 381  CAS    MIN II 10.8.
V 388  CAS    WOLF 47 (MU=0.82", P=80G). CA KOMOHEHT
              POKO ECKO AP (RO=294"), PKM
              KOMOHEHTOM KOTOPO BETC BEA
              WOLF 46=BD+61G 195 (9.4) CEKTPAHOO
              KACCA DM2./FAINT COMPONENT OF A WIDE PHY-
              SICAL PAIR (P=294") THE BRIGHT COMPONENT OF
              WHICH IS THE DM2 STAR WOLF 46=BD+61G 195
              (9.4).
V 392  CAS    MIN II 14.0. P VAR. MIN I=2429640.390+
              +4.54094D*E (J.D.2425300-29640); MIN I=
              =2429640.390+4.54064D*E (J.D.2429640-
              -36900)  4027!; OCE/SINCE J.D.2436900-
              CM. TA./SEE TABLE. HA/DEPTH OF MIN
              VAR?
V 394  CAS    MIN II 15.6.
V 396  CAS    MIN II 10.2.
V 399  CAS    MIN II 14.1.
V 401  CAS    MIN II 15.7.
V 402  CAS    MIN II 15.3.
V 406  CAS    MIN II 16.8.
V 410  CAS    PKA B 1938-39 . MEEHHA. HE KPACHA.
              /BRIGHT IN 1938-39. SLOW. NOT RED.
V 423  CAS    MIN II 14.3.
V 427  CAS    MIN II 13.7.
V 428  CAS    KPACHA./RED.
V 430  CAS    CEBEPH KOMOHEHT TECHO AP. KPACHA.
              /NORTHERN COMPONENT OF A CLOSE PAIR. RED.
V 434  CAS    KPACHA./RED.
V 441  CAS    P=351.2D?
V 442  CAS    D=0.025P. P VAR? OCE/SINCE 1972
              P=3.592120D.
V 444  CAS    MIN II 16.0. P VAR. MIN I=2438651.314+
              +2.224808D*E (J.D.2432850-37300); OCE
              /SINCE J.D.2437300-CM. TA./SEE TABLE.
              MEHEHE EPOA, MOET T, KHO.
              /PERIOD VARIATION MAY BE CYCLIC. CPEHE E-
              MEHT:/MEAN ELEMENTS: MIN I=2443194.258+
              +2.224773D*E.
V 445  CAS    MIN II 11.08.
V 448  CAS    MIN II 15.0.
V 450  CAS    VB A (B 17.5M:, 3.4", 188G). PBEEH PE-
              E MEHEH CMMAPHOO ECKA./RANGE
              OF COMBINED LIGHT VARIATIONS IS GIVEN.
V 459  CAS    MIN II 11.6.
V 466  CAS    B PAOHE CKOEH/IN THE REGION OF THE CLUS-
              TER NGC 457.
V 480  CAS    MIN II 14.7.
V 482  CAS    VB A (B 10.0M, F 4 V, 6", 195G; OTECK
              /OPTICAL). P=0.28292D?
V 497  CAS    B PAOHE CKOEH/IN THE REGION OF THE CLUS-
              TER IC 1848.
V 498  CAS    CM./SEE V 497 CAS.
V 499  CAS    CM./SEE V 497 CAS.
V 509  CAS    SB 2. OTOCEPA CPET C P=3 OA.
              /PULSATION OF PHOTOSPHERE WITH P=3 YEARS.
              OPHA OOOKA, BPOEHHA B 1975 .,
              TEEP BOBPAAETC K BEE./TENUOUS
              SHELL EJECTED IN 1975 IS NOW FALLING BACK TO
              THE STAR.
V 518  CAS    B PAOHE CKOEH/IN THE REGION OF THE CLUS-
              TER STOCK 2. BEA/STAR N136 (STOCK 208).
V 520  CAS    MIN II 13.1. P VAR. MIN I=2439069.559+
              +0.489832D*E (J.D.2438580-40850); OCE
              /SINCE J.D.2441150-CM. TA./SEE TABLE.
V 521  CAS    EH CKOEH/MEMBER OF THE CLUSTER NGC
              7789.
V 523  CAS    MIN II 11.34. P VAR. MIN I=2432054.555+
              +0.2336882D*E (J.D.2428545-33570)  7008!;
              MIN I=2439029.461+0.23368912D*E (J.D.
              2439000-41300)  7387!; OCE/SINCE J.D.
              2440480-CM. TA./SEE TABLE.
V 524  CAS    OH, H2O MCC/EMISSION. P=163D?, 191D?
              259D?, 620D?
V 526  CAS    HAKABATC BA KOEAH:/TWO OSCILLA-
              TIONS ARE SUPERIMPOSED: P1=0.0526D (A1=
              =0.0036M), P2=0.0396D (A2=0.0056M); P2/P1=
              =0.753.
V 527  CAS    MIN II 13.5; MIN II-MIN I=0.52P.
V 532  CAS_   V 533 CAS B PAOHE CKOEH/IN THE RE-
              GION OF THE CLUSTER NGC 7789.
V 536  CAS    P VAR. MAX=2438700.262+0.395674D*E (J.D.
              2438580-39150); MAX=2441186.333+
              +0.395683D*E (J.D.2440070-41250); OCE
              /SINCE J.D.2441500-CM. TA./SEE TABLE.
V 540  CAS    AHA OXA MAX (U)./EPOCH OF MAX (U) IS GIVEN.
V 541  CAS    MIN II 11.0.
V 542  CAS    CM./SEE V 532 CAS.
V 544  CAS    P VAR. PBEEHHE EMEHT CPABEB
              OCE J.D.2428000./ELEMENTS GIVEN IN THE
              TABLE ARE VALID SINCE J.D.2428000.
V 546  CAS    B PAOHE CKOEH/IN THE REGION OF THE CLUS-
              TER NGC 103. MIN II 14.8.
V 547  CAS    VB A (B 12.4M, M 4.5, 2.8", 93G). ACTPOMETP-
              ECKA BOHA/ASTROMETRIC BINARY (A=0.12",
              P=15.9A); MU=1.75", P=98G. AH PEE -
              MEHEH CMMAPHOO ECKA./VARIATION OF
              COMBINED LIGHT IS GIVEN.
V 551  CAS    P=45.5D?/57D.?/67.5D?.
V 554  CAS    P>=3500D? D=400D?
V 559  CAS    VB A (B 7.7M, 0.25", 34G, 1976). MIN II 7.21.
V 566  CAS    VB A (B 8.3M, 1.4", 194G, 1965).
V 569  CAS    10.0-14.7 I.
V 589  CAS    B CKOEH/IN THE CLUSTER NGC 663.
V 592  CAS    E KAPK. CTPE HEEPOECKE
              KTA ECKA C XAPAKTEPHM BPEMEHEM
              OPKA MHT./WHITE DWARF. RAPID NON-PERIO-
              DIC FLUCTUATIONS OF BRIGHTNESS ON A TIME SCALE
              OF SEVERAL MINUTES.
V 598  CAS    VB A (B 12M, 19", 0G). P=2.825D?  2560!.
V 615  CAS    CTOHK EPEMEHHOO PAOEH HA
              ACTOTE 10.5 GHZ. BOMOH CTOHK GAMMA-
               X-EH./VARIABLE RADIO SOURCE ON 10.5
              GHZ; GAMMA-AND X-RAY SOURCE?
V 627  CAS    H2O MCC/EMISSION.
V 635  CAS    4U 0115+634.SB (P=24.3162D). EPO CAPA
              /PULSAR PERIOD P=3.6136S.
V 638  CAS    AHA OXA MIN./EPOCH OF MIN IS GIVEN.
ALFA   CAS    VB A (B 14.5M, 17.6", 272G; C 13.5M, 38", 105G;
              D 8.5M, 64.4", 280G).
BETA   CAS    VB A (B 13.7M, 31.3", 243G); SB (P=27D).
               FE/H!=0.64.
GAMMA  CAS    VB A (B 11.0M, 2.2", 248G; C 13.0M, 52.2", 348G).
              B OACT HII/IN HII REGION S 185. X-CTOHK
              /X-RAY SOURCE MX 0053+60. V SIN I=310 KM/S.
DELTA  CAS    VB A (B 11.5M, 31.7", 66G). MIN II 2.75. MIN II-MIN I=
              =361D. PBEEHHE EMEHT O CX OP HKEM HE
              OTBEPEH./THE ELEMENTS GIVEN IN THE TABLE
              ARE STILL NOT CONFIRMED BY ANYONE.
IOTA   CAS    VB A (B 6.89M, 2.3", 239G; C 8.40M, 7.2", 114G).
              ACTPOMETPECKA BOHA/ASTROMETRIC BINARY
              (A=0.113", P=52.4A). MAX (V)-MAX (LAMBDA 1550)=0.4P;
              A (LAMBDA 1550)=0.40M. AH PEE MEHEH CM-
              MAPHOO ECKA KOMOHEHTOB A  B./THE RANGE
              OF TOTAL BRIGHTNESS VARIATION OF COMPONENTS A AND
              B IS GIVEN.
KAPPA  CAS    P=0.09028D, P (VR)=0.14035D  2588!; P=7D  8876!.
OMIKRO CAS    VB A (B 11.7M, 33.6", 303G). SB 1 (P=1033D);
              V SIN I=220 KM/S.
RO     CAS    OHO MEHETC B PEEAX 4.4M-5.2M V. B HO-
              PE 1945 . HAAOC EKPHOE AEHE ECKA,
              BEEC 165D,  B CEHTPE 1946 . BEA O-
              CTA CEPEH HAOEE OKOO MHMMA
              (J.D.2432070), B KOTOPOM PEBAA 320D. ATEM
              HAAC CMMETPH O'EM ECKA,  B E
              1947 . ECK BE OCT HOPMAHOO HAE-
              H  0957!. OTOPAECKE BEH MEHC
              B PEEAX 5.4M-8.3M. OCAHE CEKTPA  8878!.
              /USUALLY VARIES WITHIN THE LIMITS 4.4M-5.2M V.
              IN NOVEMBER 1945 THE PECULIAR DECREASE OF BRIGHT-
              NESS BEGAN LASTING FOR 165D AND IN SEPTEMBER
              1946 THE STAR REACHED THE MIDDLE OF THE DEEPEST
              MINIMUM (J.D.2432070) LASTING FOR 320D. THEN
              THE BRIGHTNESS BEGAN TO INCREASE SYMMETRICALLY
              AND JULY 1947 THE STAR ATTAINED ITS NORMAL BRIGHT-
              NESS  0957!. PHOTOGRAPHIC MAGNITUDES VARIED IN
              THE LIMITS 5.4M-8.3M. SPECTRUM DESCRIPTION  8878!.
B      CAS    CBEPXHOBA TXO PAE/TYCHO BRAHE'S SUPERNO-
              VA. OTECK BEH O'EKT O CX OP HE
              OTOECTBEH./STELLAR OBJECT IS NOT IDENTIFIED
              OPTICALLY UP TO NOW.
R      CEN    VB A (B 12M, 28", 218G). AHA OXA MIN I./EPOCH
              OF MIN I IS GIVEN. MIN I 0.00P, MAX I 0.23P, MIN II
              0.47P, MAX II 0.64P. <MAX I>5.8, <MAX II>6.0,
              <MIN I>11.1, <MIN II>8.3. P VAR. P=561.3D O
              /BEFORE 1918; OCE/SINCE 1918-CM. TA./SEE
              TABLE. H2O MAEP/MASER.
V      CEN    B OACT PACCEHHOO CKOEH/IN THE FIELD
              OF THE OPEN CLUSTER NGC 5662.
Z      CEN    SN 1895 (NGC 5253).
RR     CEN    MIN II 7.63. DII=0.08P. P VAR. MIN I=2424231.0910+
              +0.60568807D*E+2.31D*10**-10*E**2 (J.D.2414170-
              -33470)  0006!. TEKE EMEHT/CURRENT ELE-
              MENTS-CM. TA./SEE TABLE.
RS     CEN    A 1118-61?
RT     CEN    P VAR.
RZ     CEN    MIN II 9.4.
SS     CEN    MIN II 9.5.
ST     CEN    MIN II 11.30, DII=0.22P. MAX II (EPE/BEFORE
              MIN I) 10.65.
SU     CEN    MIN II 9.2.
SV     CEN    MIN II 9.45. DM VAR. P VAR. MIN=2433053.358+
              +1.6594795D*E-7.61D*10**-8*E**2 (J.D.2412608-
              -42097). B  0009, 5212! OTMEEH KECKE
              (32A-33.6A) MEHEH P./CYCLIC (32A-33.6A) PE-
              RIOD VARIATIONS WERE NOTED IN  0009, 5212!. OCE
              /SINCE 1978-CM. TA./SEE TABLE. B CEKTPE
              PO TA P CYG./P CYG PROFILES IN THE SPEC-
              TRUM.
SX     CEN     CPEHEO ECKA/FOR MEAN LIGHT MAX=
              =2426835+615D*E.
SY     CEN    D=0.05P.
SZ     CEN    VB. MIN II 8.7.
TX     CEN    VB? B-V:+1.39, +2.11.
TZ     CEN    KOOPHAT B TAE- O  0015!. COACHO
               0016!, HA TOM MECTE HE HAEHO BE PE
              14M. BOMOHO, KOOPHAT B  0015! OOH.
              /THE CO-ORDINATES IN THE TABLE ARE BASED ON
               0015!. ACCORDING TO  0016!, NO STAR BRIGHTER
              THAN 14M WAS FOUND IN THIS POSITION. THE CO-ORDI-
              NATES IN  0015! MAY BE IN ERROR.
UW     CEN    K TOK./IR EXCESS. B MAX-OPAB-
              HE KOEAH, P-42D  8832!./IN MAX VARIES SE-
              MIREGULARLY, P-42D  8832!.
UZ     CEN    VB A (B 13.8M, 4", 191G). MAX II=2440746.2+
              +2.35529D*E.
VW     CEN    VB A (B-15M?, -8", -180G). B-V:+1.01, +1.71.
               A/H!=0.3.
VZ     CEN    MIN II 8.4.
WX     CEN    <B-V>=+0.45, <U-B>=-0.72. B  5314! PEOE-
              HO OTOECTBEHE C PEHTEHOBCKO HOBO
              CEN X-2, XOT OTECKO BCEHO AKTBHO-
              CT HE HAAOC./PROPOSED AS AN OPTICAL
              COUNTERPART OF THE TRANSIENT X-RAY SOURCE
              CEN X-2  5314!, THOUGH NO OPTICAL BURSTS WERE
              OBSERVED.
WZ     CEN    MIN II 14.2.
ZZ     CEN    VB C (A 9.4M, B9; B 10.8M, 8", 314G; C=ZZ CEN,
              9", 259G; D=AA CEN, 9", 110G).
AA     CEN    VB D (CM./SEE ZZ CEN).
AB     CEN    D=0.05P.
AP     CEN    AHA OXA MIN./EPOCH OF MIN IS GIVEN.
AS     CEN    MIN II 13.2.
AV     CEN    MIN II 14.1.
AZ     CEN    OPMA KPBO ECKA MEHETC./THE SHAPE OF
              THE LIGHT CURVE VARIES.
BD     CEN    MIN II 10.7.
BF     CEN    B OACT PACCEHHOO CKOEH/IN THE FIELD
              OF THE OPEN CLUSTER NGC 3766. MIN II 8.8.
BG     CEN    MIN II 12.3.
BH     CEN    B PACCEHHOM CKOEH/IN THE OPEN CLUSTER
              IC 2994. MIN II 8.8.
BI     CEN    DS=2.
BK     CEN    P2=2.236D, A1=0.54M, A2=0.22M  8835!.
BV     CEN    CPEH K ME BCKAM <=149.4D  7301!.
              EMEHT B TAE COOTBETCTBT MAX ATMEH-
              HO KPBO ECKA, FI (MIN)=0.25P. PEE AT-
              MEHHO EPEMEHHOCT 12.8-13.3./THE MEAN CYC-
              LE BETWEEN OUTBURSTS <=149.4D  7301!. THE TABULA-
              TED ELEMENTS CORRESPOND TO MAX OF THE ECLIPSING
              LIGHT CURVE, FI (MIN)=0.25P. THE RANGE OF THE ECLIP-
              SING VARIABILITY IS 12.8-13.3.
CN     CEN    MIN II 13.3.
DI     CEN    MIN II 12.3, MIN II-MIN I=0.494P, DII=0.08P:.
DT     CEN    KPACHA./RED.
DX     CEN    P-BEA B APE./THE P STAR IN A PAIR.
DY     CEN    BCE H B CEKTPE OEH CAE. HET K
              TKA. OCAHE OTOMETPECKOO OBEE-
              H BHE OX MIN  8836!./ALL SPECTRAL LINES
              ARE VERY WEAK. NO IR EXCESS. THE PHOTOMETRIC
              BEHAVIOUR OUTSIDE MAJOR MIN OF DESCRIBED IN
               8836!.
EP     CEN    MIN II 11.5.
EU     CEN    CM./SEE DX CEN.
GI     CEN    B OACT APOBOO CKOEH/IN THE FIELD OF
              THE GLOBULAR CLUSTER NGC 5286.
IQ     CEN    D=0.04P.
IW     CEN    MIN II 12.1.
IX     CEN    B OACT PACCEHHOO CKOEH/IN THE FIELD
              OF THE OPEN CLUSTER NGC 3706.
IY     CEN    B OACT PACCEHHOO CKOEH/IN THE FIELD
              OF THE OPEN CLUSTER IC 2944.
IZ     CEN    <B-V>=1.7.
KK     CEN    B-V:+1.08, +1.62.
KM     CEN    MIN II 13.3.
KN     CEN    B-V:+1.36, +1.75.  A/H!=0.2.
KQ     CEN    CMEHE P PA EPO/ALTERNATING PE-
              RIODS 136D, 159D.
KT     CEN    B-V:+0.46. MIN II 12.72. MIN II-MIN I=0.392P
              (J.D.2441686-721); HAAETC BEHE H
              AC/APSIDAL MOTION IS OBSERVED  8094!.
KY     CEN    MIN II 13.3.
KZ     CEN    B-V:+0.30, +0.72.
LL     CEN    MIN II 13.1.
LR     CEN    MIN II 12.30.
LT     CEN    MIN II 9.6.
LU     CEN    EPO, BOMOHO, HAO BOT./THE PERIOD MAY
              BE TWICE LONGER.
LV     CEN    B-V:+1.3, +1.7.
LW     CEN    MIN II 9.6. CM./SEE IY CEN.
LX     CEN    MIN II 13.55.
LZ     CEN    MIN II 8.50.
MM     CEN    MIN II 12.7.
MN     CEN    MIN II 8.7. VB A (B 10.9M, 7", 147G).
MP     CEN    MIN II 10.0.
MQ     CEN    MIN II 10.1.
MR     CEN    MIN II 10.5.
MV     CEN    MIN II 14.6.
MY     CEN    B-V:+1.58, +1.94.
NO     CEN    MIN II 14.2.
NP     CEN    MIN II 10.2.
NY     CEN    MIN II 11.9.
OO     CEN    <B-V>=1.84.
OP     CEN    MIN II 13.8.
OU     CEN    MIN II 10.9.
OV     CEN    MIN II 11.0.
OX     CEN    MIN II 14.3.
QS     CEN    D=0.03P.
QT     CEN    MIN II 13.4.
QY     CEN    <B-V>=2.16.
QZ     CEN    P VAR? OPMA KPBO ECKA MEHETC?/THE SHAPE
              OF THE LIGHT CURVE VARIES?
V 339  CEN    VB A (B-13M, SP). B-V:+1.08, +1.47.
V 343  CEN    MIN II 13.5.
V 344  CEN    MIN II 12.3.
V 346  CEN    B OACT PACCEHHOO CKOEH/IN THE
              FIELD OF THE OPEN CLUSTER STOCK 14. MIN II 8.8.
              MIN II=2421966.835+6.32189D*E.
V 348  CEN    D=0.010P.
V 349  CEN    MIN II 14.5.
V 350  CEN    MIN II 10.3. MIN II=2430870.192+3.216906D*E.
V 351  CEN    CM./SEE AP CEN.
V 356  CEN    MIN II 15.0.
V 358  CEN    CM./SEE AP CEN.
V 365  CEN    D=0.040P.
V 373  CEN    VB A (B-4" NP).
V 377  CEN    D=0.003P.
V 379  CEN    MIN II 8.9.
V 380  CEN    MIN II 10.0.
V 383  CEN    MIN II 13.6:, MIN II-MIN I=0.609P.
V 384  CEN    MIN II 12.2. DII=0.062P. MIN II-MIN I=0.667P.
V 385  CEN    MIN II 13.0.
V 388  CEN    MIN II 15.7.
V 399  CEN    D=0.020P. MIN II 13.1.
V 405  CEN    P VAR, 30D-40D.
V 412  CEN    VB A (B 59", 266G).
V 419  CEN    P VAR. MAX=2428099.25+5.50713D*E
              (J.D.2428099-33573); OCE/SINCE
              J.D.2434900-CM. TA./SEE TABLE.
V 420  CEN    B-V:+0.45, +0.97. P VAR. KBAPATH EH:
              /NONLINEAR TERM:-0.000090D*E**2.
V 427  CEN    AHA OXA MIN./EPOCH OF MIN IS GIVEN.
V 436  CEN    SB (P=0.0669D). OTOMETPECK P BO BPEM
              CBEPXMAKCMMOB/PHOTOMETRIC P DURING SUPER-
              MAXIMA 0.06383D  8838!. CTPE KOEAH B
              CBEPXMAKCMME/RAPID OSCILLATIONS IN SUPER-
              MAXIMA DM-0.002M, P-19.6S  8049!.
V 440  CEN    D=0.033P. MIN II BOMOEH/IS POSSIBLE.
V 443  CEN    D=0.025P.
V 491  CEN    MHMM OEH OCK; TECH CTHK?
              /VERY FLAT MINIMA; CLOSE COMPANION?
V 495  CEN    D=0.042P. MIN II 10.6. MIN II-MIN I=0.520P.
V 496  CEN    BOMOH EH PACCEHHOO CKOEH/POSSI-
              BLE MEMBER OF THE OPEN CLUSTER NGC 4755.
              B-V:+1.02, +1.33.
V 498  CEN    P, BOMOHO, BBOE MEHE./P MAY BE TWICE
              SHORTER.
V 499  CEN    (K-B)2=0.23.
V 504  CEN    HAATC TAKE OPABHE KOEA-
              H, P1-130D, P2-411D  8836!./SEMIREGULAR
              VARIATIONS (P1-130D, P2-411D) ARE ALSO OBSER-
              VED  8836!.
V 508  CEN    MIN II 13.2.
V 526  CEN    DM VAR. P VAR. MAX=2425707.540+0.56153D*E
              (1929-1930); B HTEPBAE/DURING 1931-1940
              -CM. TA./SEE TABLE.
V 532  CEN    BEA/STAR 1  9078!. X-CTOHK/X-RAY SOURCE
              3A 1431-409.
V 544  CEN    2AS E 1440-39?  5962!.
V 545  CEN    BEHA B MAX?MAGNITUDE IN MAX VAR (12.6-
              -14.5), P=1800D?
V 553  CEN     FE/H!=-0.1;  C/FE!=+0.8.
V 565  CEN    MIN II 13.9. HE CKEH T RR/TYPE RR IS
              NOT EXCLUDED (P=0.238072D).
V 574  CEN    SP BEA B APE./SP STAR OF A PAIR.
V 585  CEN    MIN II 13.0.
V 592  CEN    CPEH ECK/MEAN BRIGHTNESS VAR.
V 593  CEN    BOMOH EH PACCEHHOO CKOEH/PO-
              SSIBLE MEMBER OF THE OPEN CLUSTER STOCK 16.
              MIN II 11.2.
V 594  CEN    V 133 (OMEGA CEN); HE EH CKOEH./NON-MEM-
              BER OF THE CLUSTER. MIN II 14.4.
V 606  CEN    MIN II 9.8.
V 607  CEN    MIN II 14.1.
V 608  CEN    MIN II 13.1.
V 609  CEN    MIN II 13.6.
V 615  CEN    MIN II 14.0.
V 617  CEN    MIN II 13.8:.
V 619  CEN    B OACT PACCEHHOO CKOEH/IN THE
              FIELD OF THE OPEN CLUSTER NGC 5316.
V 621  CEN    D=0.05P.
V 624  CEN    MIN II 14.9.
V 625  CEN    MIN II 15.0.
V 627  CEN    D=0.02P.
V 628  CEN    MIN II 13.2.
V 630  CEN    MIN II 14.2. D=0.06P.
V 635  CEN    MIN II 13.9.
V 636  CEN    MIN II 8.8.
V 644  CEN    BO BPEM OCAEH ECKA 1951 . HA-
              AC CEKTP OOOK  2128!. COACHO
               6763!, BOMOEH T E C OEH OM
              EPOOM./DURING THE FAINT PHASE IN 1951 THE
              SHELL SPECTRUM WAS OBSERVED  2128!. TYPE E
              WITH A VERY LONG PERIOD IS POSSIBLE  6763!.
V 645  CEN    PROXIMA CEN=ALFA CEN C. MU=3.809", P=281.7G. C-
              TOHK MKOO PEHTEHOBCKOO EH.
              /SOFT X-RAY SOURCE.
V 646  CEN    D=0.022P. MIN II 9.1.
V 662  CEN    P-2.48D /OR 2.95D.
V 672  CEN    MIN II 11.4-11.6 (VAR).
V 673  CEN    HA/DEPTH OF MIN II 0.05M.
V 674  CEN    EKT AKO:/BLAZHKO EFFECT: =29.5D.
              0.15P<=M-M<=0.23P.
V 676  CEN    MIN II 12.5.
V 677  CEN    MIN II 11.6.
V 678  CEN    MIN II 10.6.
V 679  CEN    9.8"P, 1.1"N OT/FROM CPD-62G2167. PACOOE-
              HA HA KPA TEMHOO OAKA B PKO TMAHHO-
              CT, BEC ACT IC 2944, B OACT
              OEH EHOO PACCEHHOO CKOEH. C 1950
              O 1954 . OCAEA HA 2.5M. OBOHO KPAC-
              HA. KPAHPOBAHE KPAEM TEMHO TMAHHOCT?
              /THE STAR IS AT THE EDGE OF A DARK CLOUD IN A
              BRIGHT NEBULA, A PART OF IC 2944, IN THE FIELD
              OF A VERY POOR OPEN CLUSTER. SINCE 1950 TILL
              1954 FADED BY 2.5M. RATHER RED. "SCREENING"
              BY THE EDGE OF A DARK NEBULA?
V 682  CEN    K TOK./IR EXCESS.
V 684  CEN    HA/DEPTH OF MIN II 0.05M.
V 685  CEN    MIN II 9.5.
V 686  CEN    T RV HE CKEH./RV TYPE IS NOT EXCLUDED.
V 687  CEN    MIN II 14.1. DII=0.12P. MIN II-MIN I=0.580P.
V 688  CEN    MIN II 12.7.
V 689  CEN    MIN II 12.1.
V 690  CEN    HA/DEPTH OF MIN II 0.03M.
V 692  CEN    MIN II 11.6. MIN II-MIN I=0.481P.
V 701  CEN    VB? D=0.026P. MIN II 9.1.
V 704  CEN    K TOK./IR EXCESS.
V 716  CEN    MIN II 6.21.
V 742  CEN    MIN II 10.1.
V 743  CEN    (K-B)2=0.20. EMEHT, OT CTO E XO-
              POO OBETBOPE HAEHM:/ELE-
              MENT ALMOST AS WELL SATISFACTORY: MAX=
              =2439243.6465+0.10222560D*E.
V 745  CEN    MIN II 9.6.
V 746  CEN  = V 467 CEN. HA KAPTE OOHAEHA KAK
              V 467 CEN./MARKED AS V 467 CEN IN THE CHART.
V 747  CEN    MIN II 10.05.
V 748  CEN    B-V:+0.31, +1.21; U-B: -0.66, -0.21. D=
              =0.106P. KA HALFA B MCC. BHE ATMEH-
              KOEAH ECKA HA 0.05M-0.1M A BPEM
              OT HECKOKX HE O HECKOKX HEE
              (BEPOTHO, HEPABHE)  6968!./NARROW
              HALFA EMISSION. OUTSIDE ECLIPSES SHOWS VARIATI-
              ONS BY 0.05M-0.1M DURING SEVERAL DAYS OR SE-
              VERAL WEEKS (PROBABLY IRREGULARLY)  6968!.
V 752  CEN    MIN II 9.61. DI=DII=0.047P.
V 753  CEN    (K-B)2=0.20. B OACT PACCEHHOO CKOE-
              H NGC 3960; BEPOTHO, HE EH CKOEH
              BOMOEH T DSCT./IN THE FIELD OF THE OPEN
              CLUSTER NGC 3960; PROBABLY NONMEMBER. TYPE
              DSCT IS POSSIBLE.
V 754  CEN    HEOK/SLIGHT MIN II.
V 755  CEN    B OHOM MEKE./IN THE COALSACK.
V 756  CEN    CM./SEE V 755 CEN. B CEKTPE-H BCO-
              KOO BOEH OVII, OVIII, CV. BOMOEH
              T WR  7372!./HIGH EXCITATION LINES (OVII,
              OVIII, CV) ARE PRESENT IN THE SPECTRUM. WR
              TYPE IS POSSIBLE  7372!.
V 757  CEN    MIN II 8.6.
V 758  CEN    D=0.07P. MIN II 9.15.
V 759  CEN    MIN II 7.56.
V 761  CEN    K TOK./IR EXCESS.
V 763  CEN    VB A (B 13M, 7", 163G).
V 766  CEN    VB A (B 10.01M, BOIBP, 9", 318G). K TOK.
              /IR EXCESS.
V 767  CEN    VB A (B 11.52M, 21", 350G).
V 768  CEN    BOMOH/POSSIBLE P: 60D-80D.
V 770  CEN    COACHO/ACCORDING TO  7570!, CONST?
V 772  CEN    B OACT PACCEHHOO CKOEH/IN THE REGI-
              ON OF THE OPEN CLUSTER IC 2944.
V 775  CEN    BOMOEH T EB. OK MIN II./EB TYPE
              IS POSSIBLE. DEEP MIN II.
V 777  CEN    OK/DEEP MIN II.
V 779  CEN    CEN X-3 (3U 1118-60). <B-V>: +1.04;
              <U-B>: -0.08. MIN II 13.39. PORB VAR. OPMA
              KPBO ECKA MEHETC. AHA OXA MIN I.
              OX MIN II COBAAT C MOMEHTAM ATMEH
              PEHTEHOBCKOO CTOHKA. HAATC M-
              C PEHTEHOBCKOO EH C PPULS=
              =4.834477S (OXA J.D.2442785.3); PPULS
              MEHAETC  7612!. CTPX OTECKX
              KOEAH HE OHAPEHO./THE SHAPE OF THE
              LIGHT CURVE VARIES. EPOCH OF MIN I IS GIVEN.
              EPOCHS OF MIN II COINCIDE WITH THE MOMENTS OF
              X-RAY ECLIPSES. X-RAY PULSES ARE OBSERVED
              WITH PPULS=4.834477S (EPOCH J.D.2442785.3);
              PPULS DECREASES  7612!. NO RAPID OPTICAL OS-
              CILLATIONS WERE FOUND.
V 783  CEN    B-V: +0.35.
V 784  CEN    OEH KPACHA./VERY RED.
V 788  CEN    MIN II 5.90.
V 790  CEN    VB B (A 4.52M; 60", 343G).
V 791  CEN    B PAOHE APOBOO CKOEH./IN THE REGION
              OF GLOBULAR CLUSTER OMEGA CEN (NGC 5139). HE EH
              CKOEH./CLUSTER NON-MEMBER.
V 795  CEN    VB A (B 12.29M, 33.9", 170G; C 12.79M, 36",
              220G).
V 801  CEN    4U 1145-61=2S 1145-619. BOKP ABHOO
              KOMOHEHTA-OOKA MAO OTHOCT, PAC-
              PAC CO CKOPOCT 1800 KM/C./PRIMA-
              RY COMPONENT HAS A LOW DENSITY ENVELOPE EX-
              PANDING WITH THE VELOCITY OF 1800 KM/S.
              V SIN I=290 KM/S. X-RAY PULSAR (P=291.8S
               8883!). MAX (X)=2442519.5+187.5D*E  8881!.
V 803  CEN    OEH OPA EHA BOOPOOM EEBA
              BEA./EXTREMELY HOT HYDROGEN-DEFICIENT HE-
              LIUM STAR.
V 807  CEN    VB (9.9M, 10.1M, 0.4", 258G, 1931). KAKO KOM-
              OHEHT MEHETC-HEBECTHO./IT IS NOT
              KNOWN WHICH OF THE COMPONENTS VARIES.
V 810  CEN    EH CKOEH/MEMBER OF THE CLUSTER STOCK
              14.
V 813  CEN    CM./SEE V 791 CEN. V 65 (NGC 5139).
V 814  CEN    CM./SEE V 791 CEN. V 78 (NGC 5139).
              MIN II 14.165:. ABH KOMOHEHT, BOMO-
              HO, MEHET ECK  8884!./PRIMARY COMPONENT
              IS PROBABLY INTRINSICALLY VARIABLE  8884!.
V 816  CEN    EKPHA MAHTHA OMEBA BEA.
              AHA OXA MAX (B)./PECULIAR MAGNETIC HOL-
              MIUM STAR. EPOCH OF MAX (B) IS GIVEN. HA OC-
              HOBHOE KOEAHE HAKABATC KOEAH
              C ACTOTAM:/PRIMARY OSCILLATION IS SUPERIM-
              POSED BY THE OSCILLATIONS WITH FREGUENCIES:
              F2=4.9229, F3=4.7343, F4=4.9317  2591!.
V 820  CEN     FE/H!=-2.5; VR=+260 KM/S.
V 822  CEN    CEN X-4.
V 825  CEN    CM./SEE V 791 CEN. V 2 (NGC 5139).
V 826  CEN    CM./SEE V 791 CEN. V 129 (NGC 5139).
BETA   CEN    VB A (B 4.1M, 1.3", 251G, 1960). SB 1 (P=352D
               8887!. MTEPOHOCT; HOA OCTOHCT-
              BO ECKA  8215!./MULTIPERIODICITY; SOMETIMES
              BRIGHTNESS IS CONSTANT  8215!. MKOE PEHTEHOB-
              CKOE EHE./SOFT X-RAY SOURCE.
DELTA  CEN    VB A (B 4.8M, 68.6", 325G; C 6.5M, 16.6", 227G).
EPSILO CEN    VB A (B 13.0M, 36.0", 158G). MEETC BTOPOE KO-
              EAHE ECKA C AMTO 0.0034M  EMEH-
              TAM:/THERE IS A SECONDARY LIGHT OSCILLATION WITH
              THE AMPLITUDE OF 0.0034M AND ELEMENTS: MAX=
              =2441041.058+0.17696D*E.
ETA    CEN    VB A (B 13.5M, 5.6", 270G, 1897); SB?
MU     CEN    VB A (B 13.63M, 48", 128G).
OMIKRO 1 CEN  VB A (B 11.4M, 13.5", 125G).
T      CEP    P VAR. MAX=2414252+386.05D*E (J.D.2406900-
              -20490); MAX=2431086+394.93D*E (J.D.2420490-
              -32900); MAX=2440262+379.22D*E (J.D.2432900-
              -42200); OCE/SINCE J.D.2442200 MAX=2444171+
              +392.7D*E. B TAE AHO CPEHEE HAEHE
              EPOA./MEAN VALUE OF THE PERIOD IS GIVEN IN
              THE TABLE. SIO MAEP/MASER.
U      CEP    VB A (B 11.83M, 13.9", 62G; C 12.3M, 23.0", 318G).
              0.010P<=D<=0.040P. MIN II 6.93. P VAR. MIN I=
              =2407890.3346+2.4928551D*E+5.15D*10**-9*E**2
              (J.D.2388855-2440790)  6468!; AHA MEHE-
              H EPOA B TOM HTEPBAE CM. TAKE B
               7395!/ANALYSIS OF PERIOD VARIATIONS IN THIS IN-
              TERVAL SEE ALSO IN  7395!; MIN I=2441395.3604+
              +2.4931048D*E (J.D.2440790-41600); MIN I=
              =2441679.5716+2.4930432D*E (J.D.2441600-950);
              MIN I=2443753.7982+2.4930679D*E (J.D.2442100-
              -43800); OCE/SINCE J.D.2444000-CM. TA.
              /SEE TABLE. OPMA KPBO ECKA  H
              MHMMOB MEHTC./SHAPE OF THE LIGHT CURVE
              AND DEPTH OF MINIMA VARY. ECK CTHKA (G8)
              MEHETC COPAECK. P OPAH OH TE-
              PET MACC. OTOK BEECTBA, CTPEMC
              K ABHOM (B7) KOMOHEHT, OPAET BOKP
              HEO AOBOE KOO  CK  8889!./BRIGHT-
              NESS OF THE SECONDARY (G8) VARIES SPORADICALLY.
              SUBGIANT BRIGHTENING ACCOMPANIES ERUPTIVE MASS
              TRANSFER. THE GASEOUS STREAM MOVING TO THE PRI-
              MARY (B7) COMPONENT FORMES AROUND IT GASEOUS
              RING OR DISC  8889!.
W      CEP    HA MEEHHE KOEAH ECKA C =2000D
              HAKABATC KOEAH C P=350D./SLOW OS-
              CILLATIONS WITH =2000D ARE SUPERIMPOSED BY OS-
              CILLATIONS WITH P=350D.
X      CEP    OH MCC?/EMISSION?
RS     CEP    D=0.039P. P VAR. MIN=2417140.469+12.419925D*E
              (J.D.2410000-31000)  2431!; OCE/SINCE J.D.
              2431000-CM. TA./SEE TABLE.
RZ     CEP    P VAR. MAX=2411640.654+0.308697D*E (J.D.
              2411640-15000); MAX=2417144.620+0.3086203D*E
              (J.D.2415600-20200); MAX=2421175.611+
              +0.3086699D*E (J.D.2421175-23000); MAX=
              =2423768.475+0.3086918D*E (J.D.2423000-31700);
              MAX=2433768.493+0.3086383D*E (J.D.2433700-
              -38300)  8890!; MAX=2438207.938+0.308645D*E
              (J.D.2438200-39040)  3879!; MAX=2440834.579+
              +0.3086735D*E (J.D.2440800-42640)  8890!;
              OCE/SINCE J.D.2442640-CM. TA./SEE TABLE.
              OPMA KPBO ECKA  AMTA A MEHTC
              C EPOOM EKTA AKO PB/SHAPE OF THE
              LIGHT CURVE AND THE AMPLITUDE A VARY WITH THE
              BLAZHKO EFFECT PERIOD PB=96.8*P0=29.88D;
              MIN A=2441464.147+29.88D*N  8891!. BOMOHO
              OOEPOECKOE MEHEHE P0 C EPOOM
              OKOO 50 ET./LONG PERIOD VARIATION OF P0 WITH
              A PERIOD-50 YEARS IS POSSIBLE. DS=6.
SS     CEP    CPEH ECK MEHETC C KAM OT HECKO-
              KX COTEH O TC HE./MEAN BRIGHTNESS VA-
              RIES WITH CYCLES FROM SOME HUNDREDS TO THOUSANDS
              DAYS.
SU     CEP    MIN II 10.6.
SV     CEP    K TOK/IR EXCESS.
SX     CEP    B PAOHE TMAHHOCT/IN THE REGION OF THE NEBULA
              NGC 7023.
SY     CEP    MIN II 12.70. P VAR?
SZ     CEP    VB A (B 12.3M, 24.9", 263G). S4/6 E.
TT     CEP    VB A (B 17.0M, 8", 160G).
TY     CEP    AHA OXA MIN I./EPOCH OF MIN I IS GIVEN.
UZ     CEP    P VAR. MAX=2440969+297.68D*E (J.D.2414000-
              42000); OCE/SINCE J.D.2440000-CM. TA.
              /SEE TABLE.
VV     CEP    VB (0.05", 174G, 1950)? 0.066P<=D<=0.091P;
              0.040P<=D<=0.077P. HA ATMEH:/DEPTH OF
              ECLIPSES: 2.30M (LAMBDA 3500 A), 1.9M (U), 0.4M (B).
              M-KOMOHEHT-TA SRC:/M-COMPONENT IS OF
              SRC TYPE: MAX=2443045+118.37D*E  8698, 8894!;
              A(V)<=0.33M. OTMEEH TAKE KOEAH ECKA
              C P=/LIGHT OSCILLATIONS ARE ALSO NOTED WITH P=
              =58D  8895!, 25D AND 150D  8896!. B-KOMOHEHT
              TAKE, BOMOHO, MEHET ECK/B-COMPONENT
              MAY BE ALSO AN INTRINSIC VARIABLE  2416!. AOBE
              OTOK. CHOE EPEMEHHOE MAHTHOE OE./
              /GASEOUS STREAMS. STRONG VARIABLE MAGNETIC FIELD.
VW     CEP    VB A (B 10.3M, A=0.51", P=30.45A  8897!); MU ALFA=
              =+0.0899S, MU DELTA=+0.560". MIN II 7.56. OPMA KPBO
              ECKA  HA MIN I  MIN II MEHTC./SHA-
              PE OF THE LIGHT CURVE AND DEPTHSOF MIN I AND MIN II
              VARY. P VAR. MIN I=2433483.4257+0.27831758D*E+
              +0.050D*COS 0.004813G*(E-4700) (J.D.2424763-
              -41200)  6483!; OCE/SINCE J.D.2441000-CM
              TA./SEE TABLE. CCEOBAHE MEHEH EPO-
              A CM. TAKE/PERIOD CHANGE STUDY SEE ALSO IN
               8899!. X-CTOHK./X-RAY SOURCE.
VZ     CEP    MIN II 9.93.
WX     CEP    MIN II 9.14; DI=0.01P, DII=0.00P.
WY     CEP    MIN II 11.5. P VAR  2545!.
WZ     CEP    MIN II 11.9.
XX     CEP    MIN II 9.26. P VAR. MIN I=2425096.449+2.337340D*E
              (J.D.2414930-30000); MIN I=2441539.4917+
              +2.3373059D*E (J.D.2430000-42300)  8902!. OCE
              /SINCE J.D.2441500-CM. TA./SEE TABLE.
XY     CEP    MIN II 10.10. P VAR?
XZ     CEP    MIN II 8.43.
ZZ     CEP    VB A (B 10.2M, A2 P, 3.6", 202G; C 10.87M, A5V,
              20.6", 219G). MIN II 8.74.
AH     CEP    MIN II 7.03. HA MHMMOB MEHETC/DEPTH
              OF MINIMA VARIES. P VAR. MIN I=2434989.3702+
              +1.7747274D*E (J.D.2415500-35000)  3604!;
              OCE/SINCE J.D.2434900-CM. TA.:/SEE TAB-
              LE:+3.12D*10**-9*E**2.
AI     CEP    MIN II 9.48.
AN     CEP    OCE J.D.2425200 OBC ABHE  BTO-
              PHE MAKCMM  MHMM,  CPEH
              K CTA 254D./SINCE J.D.2425200 PRIMARY AND
              SECONDARY MAXIMA AND MINIMA APPEARED, AND
              MEAN CYCLE BECAME 254D.
AV     CEP    D<=0.04P.
BB     CEP    D=0.050P.
BE     CEP    MIN II 13.0.
BF     CEP    P VAR. MAX=2437236+426.11D*E (J.D.2423600-
              37300); MAX=2441665+442.3D*E (J.D.2437300-
              42500); OCE/SINCE J.D.2442500-CM. TA.
              /SEE TABLE.
BH     CEP    HOA CHE AOEOOHE OCAEH
              ECKA./SOMETIMES STRONG ALGOL-LIKE LIGHT WEAKE-
              NINGS ARE OBSERVED.
BO     CEP    CM./SEE BH CEP.
CO     CEP    MIN II 12.6; MIN II-MIN I=0.552P; DII=0.080P.
CP     CEP    P VAR?
CQ     CEP    MIN II 9.03. OPMA KPBO ECKA  HA M-
              HMMOB MEHTC. COACHO  7401! 28/29
              MAPTA 1969 . HA AE 0.56P HAAOC MEH-
              EHE ECKA HA 0.1M, A ATEM CTPA BC-
              KA HA 0.35M U, 0.13M B, 0.14M V./SHAPE OF THE
              LIGHT CURVE AND DEPTH OF MINIMA VARY. ACCORDING
              TO  7401! ON 1969 MARCH 28/29 ON THE PHASE
              0.56P A LIGHT DECREASE BY 0.1M WAS OBSERVED AND
              THEN A RAPID FLARE BY 0.35M U, 0.13M B, 0.14M V.
              P VAR. KBAPATH EH:/NONLINEAR TERM:
              -10**-9*E**2.
CR     CEP    P VAR. MAX=2436846.94+6.23318D*E (J.D.2415000-
              -30000)  3157!; OCE/SINCE J.D.2430000-CM.
              TA./SEE TABLE.
CV     CEP    S7/1.5. CPEH BEHA MEHETC C KOM
              -2000D  0159!./MEAN BRIGHTNESS VARIES WITH A
              CYCLE-2000D  0159!.
CW     CEP    VB A (B 12.29M, 20", 310G). MIN II 8.01; MIN II-
              -MIN I=0.478P (1972 G.). EMEHT COEPAT C-
              HCOAH EH:/THERE IS A SINUSOIDAL TERM
              IN THE ELEMENTS:+0.0250D*SIN (0.0626G*E-28.3G).
              BEHE H AC C P=43 ./APSIDAL MOTION
              WITH P=43A.
CX     CEP    MIN II 12.16.
CY     CEP    MIN II 16.5.
DD     CEP    P VAR. MAX=2427960+167.6D*E (J.D.2427900-
              -30000); MAX=2429968+173.0D*E (J.D.2429900-
              -33600); OCE/SINCE J.D.2433600-CM. TA.
              /SEE TABLE.
DH     CEP    B OACT CKOEH/IN THE REGION OF THE CLUSTER
              NGC 7380. BPAEHE H AC C P=2.6 .
              /APSIDAL MOTION WITH P=2.6A  0165!.
DK     CEP    MIN II 12.4.
DL     CEP    MIN II 12.7.
DO     CEP    VB B (A 9.87M, M4V; A=2", 4, P=44.78A, E=0.408);
              MU=0.852", P=242.6G.
DP     CEP    MIN II 14.4.
DQ     CEP    MTEPOHOCT:/MULTIPERIODICITY: P0=
              =0.12420D:  8137!, P1=0.061177D  8914!.
DX     CEP    P VAR. MAX=2430603.712+0.5260395D*E (J.D.
              2415700-31000)  0001!; OCE/SINCE J.D.
              2431000-CM. TA./SEE TABLE. DS=7.
DY     CEP    MIN II 11.8.
EE     CEP    A VAR?
EF     CEP    MIN II 12.6. P VAR?
EG     CEP    MIN II 9.61. P VAR. MIN I=2439774.3322+
              +0.54462091D*E (J.D.2415200-41000)  0001!;
              OCE/SINCE J.D.2441000-CM. TA./SEE TABLE.
EH     CEP    B TEMHOM OAKE  HO TMAHHOCT
               CKOEH/IN THE DARK CLOUD NEAR THE DIFFUSE
              NEBULA AND THE CLUSTER NGC 7023.
EI     CEP    MIN II 7.98.
EK     CEP    MIN II 8.06; MIN II-MIN I=0.545P (1965). MIN II=
              =2439022.8484+4.427797D*E  8160!. BPAEHE
              H AC/APSIDAL MOTION (P=4700A+-600A)
               8923!.
EL     CEP    P VAR.
EM     CEP    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              NGC 7160. VB A (A 12.8M, 19.8", 281G; B 7.9M,
              62.5", 146G). MIN II 7.16. OPMA KPBO ECKA
               HA MHMMOB MEHTC./SHAPE OF THE
              LIGHT CURVE AND DEPTH OF MINIMA VARY.
EO     CEP    MIN II 12.3.
EP     CEP    B CKOEH/IN THE CLUSTER NGC 188. MIN II 17.0.
EQ     CEP    B CKOEH/IN THE CLUSTER NGC 188. MIN II 16.7.
ER     CEP    B CKOEH/IN THE CLUSTER NGC 188. MIN II 16.27.
ES     CEP    B CKOEH/IN THE CLUSTER NGC 188. MIN II 15.8.
              P VAR. MIN I=2439082.238+0.34468D*E (J.D.
              2438480-39090); MIN I=2439236.501+0.34264D*E
              (J.D.2439090-39280); MIN I=2439594.548+
              +0.34250D*E (J.D.2439400-39600); OCE/SINCE
              J.D.2439600-CM. TA./SEE TABLE. A VAR.
EX     CEP    MIN II 11.6.
EY     CEP    MIN II 10.4.
EZ     CEP    P VAR. MAX=2416803.627+0.378990D*E (J.D.
              2415400-20000)  0001!; OCE/SINCE J.D.
              2420000-CM. TA./SEE TABLE.
FH     CEP    MIN II 12.1.
FL     CEP    D=0.02P.
FS     CEP    MIN II 12.0.
FT     CEP    VB A (B 18.3M, 5", 27G). CM./SEE FU CEP.
FU     CEP    B PAOHE HO TMAHHOCT  CKOEH/
              /IN THE REGION OF THE DIFFUSE NEBULA AND THE CLUS-
              TER NGC 7023.
FV     CEP    CM./SEE FU CEP. HE CKEHO, TO EPEMEH-
              HA BETC ATMEHHO CCTEMO C P=0.4628D.
              /THE VARIABLE MAY BE AN ECLIPSING BINARY WITH
              P=0.4628D.
FW     CEP    CM./SEE FU CEP.
GI     CEP    MIN II 11.9.
GK     CEP    MIN II 7.35; DI=DII=0.03P; MIN II-MIN I=0.502P.
              P VAR. MIN I=2425189.526+0.9361614D*E (J.D.
              2415000-27500); MIN I=2438694.7070+
              +0.9361714D*E (J.D.2427500-38200)  0001!; OC-
              E/SINCE J.D.2438200-CM. TA./SEE TABLE.
GL     CEP    B PAOHE HO TMAHHOCT IC 1396  CKO-
              EH TR 37./IN THE REGION OF THE DIFFUSE NEBULA
              IC 1396 AND THE CLUSTER TR 37.
GM     CEP    CM./SEE GL CEP.
GP     CEP    B PAOHE OH HII S 132./IN THE REGION OF THE
              HII ZONE S 132. ETBEPTA CCTEMA, COCTOA
               ATMEHHO AP WN 6+O8-B0III: (P=6.6883D),
              ECK CBAHHO C APO O+O (P=3.4698D),
              KOTOPA MOET T TAKE ATMEHHO  -
              COAHO CCTEMO  8931!./QUADRUPLE SYS-
              TEM, CONSISTING OF A WN6+O8-B0III: ECLIPSING
              PAIR (P=6.6883D) PHYSICALLY ASSOCIATED WITH AN
              O+O PAIR (P=3.4698D); THE LATTER PAIR MAY BE ALSO
              AN ECLIPSING OR ELLIPSOIDAL VARIABLE  8931!.
GS     CEP    MIN II 10.6.
GT     CEP    MIN II 8.6.
GW     CEP    MIN II 12.00.
NK     CEP    MIN II 14.4.
HZ     CEP    CM./SEE FU CEP.
IL     CEP    VB A (B 11.91M, 7", 326G); P=2.802D?
IM     CEP    MIN II 13.6.
IO     CEP    MIN II 11.7.
IP     CEP    MIN II 12.1.
IR     CEP    VB (DM=0.0M, 0.0"-0.2"). P VAR. MAX=2431060.878+
              +2.114016D*E (J.D.2428335-31060)  0001!; OCE
              /SINCE J.D.2440900-CM. TA./SEE TABLE.
IV     CEP    VB B (A 16M; B 2.1", 191G).
IW     CEP    MIN II 13.7; MIN II-MIN I=0.52P.
IX     CEP    D=0.03P. MIN II 17.0.
KL     CEP    D=0.019P.
KP     CEP    HA/DEPTH OF MIN II 0.03M.
KV     CEP    MIN II 14.3.
KY     CEP    BCKA, BAC 65 CEKH./FLARE WITH 65
              SEC DURATION. HA MECTE BCK-OO O'-
              EKT  0001!./THERE IS A BLUE OBJECT ON THE PLACE OF
              THE FLARE  0001!.
KZ     CEP    VB (8.6M, 8.6M; 1.9", 348G). PH CEKTPAHX
              H MEHTC:/DEPTHS OF SPECTRAL LINES VARY
              P=0.212938D  6488!.
LL     CEP    MIN II 14.0.
LM     CEP    MIN II 12.8.
LP     CEP    MIN II 13.8; MIN II-MIN I=0.55P.
LO     CEP    BOCTOH KOMOHEHT BOHO BE./EASTERN
              COMPONENT OF A DOUBLE STAR.
LU     CEP    VB.
LW     CEP    HA/DEPTH OF MIN II 0.05M.
LZ     CEP    MIN II 5.63. B TAE/IN THE TABLE-P(VR)
               4627!.
MN     CEP    HA/DEPTH OF MIN II 0.08M?
MQ     CEP    MIN II 15.7.
MT     CEP    MIN II 15.5.
MX     CEP    SB (P=16.03D)  8947!.
MY     CEP    B CKOEH/IN THE CLUSTER NGC 7419. MCC/
              EMISSION OH, H2O.
MZ     CEP    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              NGC 7419.
NN     CEP    MIN II 8.52.
NR     CEP    MIN II 13.6; D=0.025P?
NS     CEP    HA/DEPTH OF MIN II 0.04M.
NW     CEP    AAH KOMOHEHT TECHO VB./PRECEEDING
              COMPONENT OF A CLOSE VB. MIN II 10.7.
NY     CEP    VB A (B 10.33M, 10", 190G); D=0.003P; SB2, E=
              =0.49; DGAMMA=GAMMA2-GAMMA1=32 KM/S   7412!.
OS     CEP    OEH KPACHA./VERY RED.
OT     CEP    MIN II 13.3.
OZ     CEP    KPACHA/RED.
PS     CEP    B PAOHE CKOEH/IN THE REGION OF THE CLUSTER
              NGC 7380. SB 2 (P=2.09168D)  5479!.
PV     CEP    CM./SEE EH CEP. B BEPHE PKO EPEMEHHO
              KOMETOOPAHO TMAHHOCT./AT THE APEX OF THE
              BRIGHT VARIABLE FAN NEBULA.
PW     CEP    CM./SEE FU CEP.
QZ     CEP    KAPTA OKPECTHOCTE, PBEEHHA B  4015! 
              BV 323, B ECTBTEHOCT BETC KAPTO
               BV 324=QZ CEP./THE MAP OF SURROUNDINGS
              GIVEN IN  4015! FOR BV 323 IS IN REALITY THE MAP
              FOR BV*324=QZ CEP. MIN II 11.9.
V 338  CEP    MIN II 9.52.
V 342  CEP    B-V=+3.6.
V 344  CEP    B-V=+4.4.
V 345  CEP    B-V=+5.0.
V 346  CEP    B-V=+4.6.
V 347  CEP    B-V=+4.5.
V 351  CEP    VB A (B 13M, 20", 135G). P VAR. MAX=2430615.57+
              +2.80511D*E (J.D.2429160-34300); MAX=
              =2435749.12+2.80556D*E (J.D.2435310-40885)
               2830!. OCE/SINCE J.D.2442020-CM. TA.
              /SEE TABLE.
BETA   CEP    VB A (A 6M, 0.204", 47.2G, 1977. 9; B 7.84M, A2V,
              13.6", 250G). SB 1 (PORB=10.893D)  6486!. P VAR.
              MAX(VR)=2417359.715+0.1904795D*E (J.D.
              2415750-22000); MAX(VR)=2422203.790+
              +0.1904844D*E+2.9440D*10**-11*E**2+3.2671D*10**-17*E**3
              (J.D.2422000-42630)  0177!. PBEEHHE B TA-
              E EMEHT PECTABT HAEH B 1967-
              69 ./ELEMENTS GIVEN IN THE TABLE SATISFY OBSER-
              VATIONS IN 1967-69.
DELTA  CEP    VB A (B 13.0M, 20.0", 285G; C 6.10M-6.37M, B7IV,
              41.0", 191G). P VAR. MAX=2393659.856+5.366438D*E
              (J.D.2372200-96900); MAX=2413960.73+
              +5.366386D*E (J.D.2396900-2414050); OCE/SIN-
              CE J.D.2414050-CM. TA./SEE TABLE. BCE HA-
              EH B HTEPBAE J.D.2373090-45000 XOPOO
              PECTABTC TAKE EMEHTAM C KBAPAT-
              HM EHOM:/ALL OBSERVATIONS IN THE INTERVAL J.D.
              2373090-45000 ARE WELL REPRESENTED ALSO BY THE
              ELEMENTS WITH A SQUARE TERM: MAX=2442756.490+
              +5.366270D*E-7D*6*10**-9*E**2  8632!.
EPSILO CEP    VB A (B 9.5M, 127.8", 15G, 1918). MTEPO-
              HOCT/MULTIPERIODICITY: P2=0.068073D
              (A2/2=0.0061M), P3=0.011823D? (A3/2=0.0022M);
              A1/2=0.0079M.
MU     CEP    VB A (B 12.3M, 19.4", 262G; C 12.7M, 41", 299G).
              HAAETC TAKE K POOTEHOCT
              4400D  8957!./THERE IS ALSO THE CYCLE WITH 4400D
              DURATION  8957!.
W      CET    S 5.5/2 E.
RR     CET     FE/H!=-1.26. P VAR. B HTEPBAE/DURING J.D.
              2417500-28820 MAX=2417501.444+0.55302577D*E;
              OCE/SINCE J.D.2433180-CM. TA./SEE TABLE.
              COACHO  8726!, PAK O-C OT EMEHTOB
               3506! MEET PMEPHO CHCOAH B C
              =2600D  AMTO 0.025D./ACCORDING TO
               8726!, THE GRAPH OF O-C DEVIATIONS FROM THE ELE-
              MENTS GIVEN IN  3506! IS APPROXIMATELY SINUSOI-
              DAL, WITH =2600D AND THE AMPLITUDE 0.025D.
RU     CET    (K-B)2=0.01. DM VAR? P VAR  2455!. MAX=
              =2426964.019+0.5863003D*E (J.D.2426500-28430)
               0181!; MAX=2434143.056+0.5862676D*E (J.D.
              2433100-35820)  2431!; OCE/SINCE J.D.
              2435820-CM. TA./SEE TABLE.
RV     CET    DS=9.
RW     CET    MIN II 10.5. P VAR. B HTEPBAE/DURING J.D.
              2426500-41000 MAX=2426585.503+0.9751814D*E
               0001!; OCE/SINCE J.D.2441000-CM. TA./SEE
              TABLE.
RX     CET    DS=5. P VAR. O/WEFORE J.D.2428500 MAX=
              =2425938.271+0.5737100D*E  3506!; OCE/SINCE
              J.D.2430000-CM. TA./SEE TABLE.
RZ     CET    DS=6.7. P VAR. B HTEPBAE/DURING J.D.
              2426585-28630 MAX=2426585.448+0.510633D*E
               3506!; TEKE EMEHT/CURRENT ELEMENTS-
              CM. TA./SEE TABLE.
SS     CET    D=0.025P. P VAR. MIN=2429321.250+2.9739509D*E
              (J.D.2427340-30700)  2419!; MIN=2430698.160+
              +2.973992D*E (J.D.2429300-36650)  3115!; OC-
              E/SINCE J.D.2440000-CM. TA./SEE TABLE.
SV     CET    MIN II 14.9.
TT     CET    MIN II 11.1.
TU     CET    D=0.043P. MIN II 10.9. MIN II-MIN I=0.478P.
              COACHO/ACCORDING TO  3564!, CEKTP/THE SPEC-
              TRUM IS K2.
TV     CET    MIN II 9.10. DII=0.03P. MIN II-MIN I=0.494P.
TW     CET    MIN II 11.14. P VAR. MIN I=2430965.595+
              +0.316852D*E (J.D.2427650-31000)  0192!; MIN I=
              =2433611.3121+0.316846D*E (J.D.2433530-615)
               0001!; OCE/SINCE J.D.2440000-CM. TA.
              /SEE TABLE.
TX     CET    B-V:+0.34, +0.37. MIN II 11.12.
TY     CET    MIN II 12.1.
UU     CET    (K-B)2=0.08. P VAR. EKT AKO?/BLAZHKO
              EFFECT?
UV     CET    VB B (A 12.45M, DM5.5 E; A=2.1", P=25A).
VV     CET    MIN II 11.0. BOMOEH TAKE T EB./EB TYPE
              IS ALSO POSSIBLE. HE CKEH T RR, C OO-
              BHHM EPOOM./RR TYPE WITH TWICE SHORTER
              PERIOD IS NOT EXCLUDED.
VX     CET    D=0.026P.
VY     CET    MIN II 11.70.
VZ     CET    ADS 1778 B (B 0.61", 122G; A=OMIKRON CET). HAA-
              TC TAKE HEOE KOEAH C XAPAKTEP-
              HM BPEMEHEM OPKA HECKOKX ACOB, HA
              KOTOPE HAKABATC ECT-THAATM-
              HTHE KOEAH  PEKE BCK, EC
              OKOO 2 MH  6492!. BOMOH E KAPK
              C AKKPEOHHM CKOM  8926!./SMALL VARIATIONS
              ARE ALSO OBSERVED ON THE TIME SCALE OF SEVERAL
              HOURS, WITH SUPERIMPOSED 10-15 MINUTE VARIATIONS
              AND RARE FLARES OF APPROXIMATELY 2 MINUTE DURATI-
              ON  6492!. A POSSIBLE WHITE DWARF WITH AN ACCRE-
              TION DISC  8926!.
WW     CET    VR VAR (P=0.160D)  4712!. HAATC CTPE
              (-10 MH) KTA ECKA  4709!./RAPID OS-
              CILLATIONS (-10 MIN) OF BRIGHTNESS ARE OBSERVED
               4709!.
WZ     CET    MIN II 11.0.
XY     CET    D=0.02P. MIN II 9.34.
YY     CET    MIN II 9.2.
ZZ     CET    HAATC OHOBPEMEHHO 4 CTAHX -
              CA:/4 STABLE OSCILLATIONS ARE OBSERVED SIMULTA-
              NEOUSLY: P1=213.132605S, P2=212.768427S, P3=
              =274.250814S, P4=274.774562S.
AA     CET    ADS 1581 A (B 7.7M VIS, SB 2, F5, 8.5", 304G).
              MIN II 6.7:. DII=0.065P.
AB     CET    ADS 1849 A (B 9.30M, 12", 293G). SB? (VR VAR,
              P=2.997814D). EPO MEHEH MAHTHOO O-
              /THE PERIOD OF MAGNETIC VARIATIONS IS 15.9D
               8932!.
AD     CET    ADS 180 A (B 10M, 3", 4G).
DELTA  CET    KBAPATH EH:/NONLINEAR TERM:
              +2.20D*10**-11*E**2.
OMIKRO CET    ADS 1778 A (B=VZ CET, 0.61", 122G). MAEP/MASER
              SIO, OH, H2O.
S      CHA    VB A (B 9.29M, 23", 134G).
T      CHA    HOA HAATC KBAEPOECKE ME-
              HEH ECKA C EPOAM 3.2323D, 3.4375D,
              4.1800D, 3.2436D, ECTBM HA POTEH
              6-26 OX. K TOK./OCCASIONALLY QUASIPE-
              RIODIC LIGHT CHANGES ARE OBSERVED WITH PERIODS
              3.2323D, 3.4375D, 4.1800D, 3.2436D OPERATING DU-
              RING 6-26 CYCLES. IR EXCESS.
Z      CHA    VB A (B 5.6"). ATMEH:/ECLIPSES: MIN=
              =2440264.68232+0.0744992195D*E+7.88D*10**-13*E**2
               8938!. D=0.065P; D=0.026P. HA MIN:/DEPTH
              OF MIN: 1.73M-2.11M B O ATMEH:/BEFORE THE
              ECLIPSE; 1.38M-1.97M B OCE ATMEH./AFTER
              THE ECLIPSE. B MIN ECKA-EPOECKE KO-
              EAH  7000!. KOEAH C P=27.7S BO BPEM
              CBEPXMAKCMMA  8049!./PERIODIC VARIATIONS
              DURING MIN LIGHT  7000!. VARIATIONS WITH P=27.7S
              DURING A SUPERMAXIMUM  8049!.
RS     CHA    EA/DM. MIN II 6.53. OH  KOMOHEHTOB-
              CPA EPEMEHHA TA DSCT. P B
              PEEAX OT 0.074D O 0.097D  8403!. DM=0.01M+
              +0.03M B CMMAPHOM ECKE./ONE OF THE COMPO-
              NENTS IS A PULSATING VARIABLE OF DSCT TYPE. P IS
              IN THE RANGE FROM 0.074D TO 0.097D  8403!. DM=
              =0.01M+0.03M IN THE COMBINED LIGHT.
RW     CHA    MIN II 14.6.
RY     CHA    MIN II 14.0.
RZ     CHA    MIN II 8.8. DII=0.11P.
SY     CHA    HAAAC KBAEPOECKA EPEMEHHOCT
              /QUASIPERIODIC VARIATIONS WERE OBSERVED. (P=
              =6.2D  4305!, P=7.6D  8946!).
TW     CHA    KBAEPOECKA EPEMEHHOCT/QUASIPERIO-
              DIC VARIATIONS (P=8.68D  4462!).
VW     CHA    K TOK./IR EXCESS.
VZ     CHA    KBAEPOECKE KOEAH/QUASIPERIODIC
              VARIATIONS (P=7.27D).
YZ     CHA    DM (MIN II)=0.4M.
CG     CHA    MIN II 14.4.
CH     CHA    MIN II 15.1.
CX     CHA    MIN II 15.5. EMEHT HEBEPEHHE./UNCERTAIN
              ELEMENTS.
CY     CHA    MIN II 14.0.
CZ     CHA    MIN II 14.6.
DD     CHA    MIN II 14.7.
DG     CHA    MIN II 14.5.
DZETA  CHA    SB.
S      CIR    MIN II 10.9.
T      CIR    MIN II 9.4.
U      CIR    P VAR. O/BEFORE J.D.2417000 MAX=2412560+
              +151D*E.
V      CIR    MIN II 11.0. COACHO/ACCORDING TO  0210!, PE-
              E MEHEH ECKA/VARIES IN THE RANGE
              10.8M-13.0M PG.
TW     CIR    MIN II 13.3.
UY     CIR    KPACHA./RED.
UZ     CIR    AHA OXA ABHOO MAX. HAOMHAET R CEN.
              /EPOCH OF MAIN MAX IS GIVEN. RESEMBLES R CEN.
              MAX I-MAX II=160D.
VX     CIR    P VAR. O/BEFORE J.D.2418000 MAX=2414360+
              +427D*E.
AQ     CIR    BOMOHO, T EW C EPOOM BBOE OE
              TAHOO./POSSIBLY EW TYPE WITH TWICE LONGER
              PERIOD.
AR     CIR    BEHA B MIN, BOMOHO, OTHOCTC K HEPAPE-
              EHHOM OT HOBO CTHK./THE MAGNITUDE IN
              MIN LIGHT POSSIBLY CORRESPONDS TO AN UNRESOLVED
              COMPANION.
AT     CIR    D=0.02D:.
AX     CIR    SB. VB? (6.5M; 6.5M; 0.5", 143G, 1913).
BD     CIR    MIN II 9.5.
BF     CIR    MIN II 8.9.
BG     CIR    MIN II 10.3.
BN     CIR    OK/DEEP MIN II. HE CKEH BBOE MEH-
               EPO./TWICE SHORTER PERIOD IS NOT EXCLUDED.
BR     CIR    CIR X-1. COACHO  8951!, O'EKT HE COBAAET
              CO BEO L (B=22.5M) HA KAPTE   2911!, A
              HAXOTC HA PACCTOH-1" K  OT HEE 
              MEET M>23.5M HA ACTHKAX IIIA-J. OCTEEH-
              HOE BOPACTAHE HTEHCBHOCT X-EH E-
              POECK OPBAETC PEKM AEHEM HTEH-
              CBHOCT. MOMEHT HAAA AEH T PECTAB-
              TC EMEHTAM T=2443292.118+16.595D*E
               2926!. AEH HTEHCBHOCT X-EH
              COPOBOATC BCKAM K  PAOE-
              H. VR (EALFA)=+250 KM/C. B 25' OT OCTATKA CBEPX-
              HOBO G 321.9-0.3./CIR X-1. ACCORDING TO  8951!,
              THE OBJECT DOES NOT COINCIDE WITH THE STAR (B=
              =22.5M) LABELLED AS L IN THE CHART IN  2911! BUT IS
              SITUATED IN-1" TO THE SOUTH OF IT AND HAS M>23.5M
              ON IIIA-J PLATES. GRADUAL INCREASE OF X-RAY INTEN-
              SITY IS PERIODICALLY STOPPED BY AN ABRUPT INTENSITY
              FALL. THE MOMENTS OF SUCH TRANSITIONS T ARE REPRE-
              SENTED BY THE ELEMENTS T=2443292.118+16.595D*E
               2926!. THE X-RAY INTENSITY FALLS ARE ACCOMPANI-
              ED BY IR AND RADIO BURSTS. VR (EALFA)=+250 KM/S. IN
              25' FROM THE SUPERNOVA REMNANT G 321.9-0.3.
TETA   CIR    VB (6.2M, 6.2M, 0.1", 96G).
T      COL    SIO MAEP/MASER.
U      COL    MIN II 10.5.
Y      COL    V2 (NGC 1851).
Z      COL    V1 (NGC 1851).
RS     COL    MIN II 9.97. DII=0.021P.
RY     COL    (K-B)2=0.10. P VAR; HEHEH EH:/NONLINEAR
              TERM:-3.38*10**-9*E**2.
RZ     COL    MIN II 11.20.
TV     COL    2A 0526-328. VB A (B 15.79M, 10", 330G). AHA
              OXA MAX KOPOTKOEPOECKX OTOMETPEC-
              KX MEHEH. CEE EMEHT OCBA-
              T, COOTBETCTBEHHO, MOMEHT MAX VR H
              AMEPOBCKO CEP  MOMEHT MAX CPABHTE-
              HO OOEPOECKO OTOMETPECKO EPE-
              MEHHOCT, CBAHHO C EHM OTOMETPEC-
              KOO  CEKTPAHOO EPOOB:/EPOCH OF MAX
              OF SHORT-TERM PHOTOMETRIC VARIATIONS IS GIVEN. THE
              FOLLOWING ELEMENTS DESCRIBE, RESPECTIVELY, MOMENTS
              OF MAX VR FOR BALMER LINES AND MOMENTS OF MAX
              FOR THE COMPARATIVELY LONG-TERM PHOTOMETRIC VARIA-
              TIONS WHICH ARE DUE TO THE BEAT PHENOMENON FOR
              THE PHOTOMETRIC AND SPECTRAL PERIODS: MAX VR=
              =2444227.631+0.228600D*E; MAX=2444191.5+
              +4.024D*E. HAATC TAKE CTPE KT-
              A ECKA (O 0.15M B)  BCK O 0.3M U
               8960!./FLICKERING UP TO 0.15M B AND FLARES UP TO
              0.3M U ARE ALSO OBSERVED  8960!.
R      COM    OH MCC/EMISSION.
S      COM    DS=8.
T      COM    OH, H2O MCC/EMISSION.
U      COM    DS=5.
V      COM    P VAR. MAX=2424518.219+0.46913844D*E (J.D.
              2420900-26900)  0218!; OCE/SINCE J.D.
              2438100-CM. TA./SEE TABLE. DS=8.
W      COM    CTOHK PAOEH/RADIO SOURCE ON 231.
X      COM    Z=0.092. OCAHE CEKTPA/SPECTRUM DESCRIP-
              TION  7415, 8966!.
Y      COM    B PAOHE APOBOO CKOEH/IN THE REGION OF
              THE GLOBULAR CLUSTER M 53 (NGC 5024).
Z      COM    CM./SEE Y COM.
RR     COM    CM./SEE Y COM.
RS     COM    B PAOHE APOBOO CKOEH/IN THE REGION OF
              THE GLOBULAR CLUSTER NGC 5053.
RT     COM    CM./SEE RS COM. A VAR; P VAR. MAX=
              =2423113.496+0.5651925D*E (J.D.2422700-
              -26450)  0222!; OCE/SINCE J.D.2438535-CM.
              TA./SEE TABLE.
RU     COM    CM./SEE Y COM.
RV     COM    CM./SEE Y COM.
RW     COM    CM./SEE CT COM. DI=0.04P; MIN II 11.56. P VAR.
              MIN I=2433040.406+0.23734705D*E (J.D.
              2419680-34550)  0185!; OCE/SINCE J.D.
              2439600-CM. TA./SEE TABLE.
RY     COM    P VAR. MAX=2425007.450+0.46894835D*E (J.D.
              2425000-27500)  3506!; MAX=2432674.390+
              +0.4689397D*E (J.D.2432600-38110)  3415!;
              OCE/SINCE J.D.2438100-CM. TA./SEE TABLE.
              (K-B)2=0.07.
RZ     COM    BOMOH EH CKOEH BOOC BEPOHK.
              /POSSIBLE MEMBER OF THE COMAE BERENICES CLUS-
              TER. MIN II 11.09; DI=0.043P, DII=0.039P. P VAR.
              MIN I=2433396.737+0.33850556D*E (J.D.2425000-
              -33300)  0226!; OCE/SINCE J.D.2433300-CM.
              TA./SEE TABLE. OPMA KPBO ECKA MEHET-
              C./SHAPE OF THE LIGHT CURVE VARIES.
SS     COM    MIN II 11.9.
ST     COM    DS=10.
SX     COM    B PAOHE APOBOO CKOEH/IN THE REGION OF
              THE GLOBULAR CLUSTER NGC 4147.
SZ     COM    CM./SEE SX COM.
TU     COM    OPMA KPBO ECKA, A  P MEHTC. B TA-
              E PBEEH CPEHE EMEHT. BOMOH
              EPO EKTA AKO 75D  3584!./SHAPE OF
              THE LIGHT CURVE, A AND P VARY. MEAN ELEMENTS
              ARE GIVEN IN THE TABLE. POSSIBLE PERIOD OF BLA-
              ZHKO EFFECT IS 75D  3584!.  FE/H!=-1.43.
UU     COM    EH CKOEH BOOC BEPOHK. MEHEH
              ECKA OCOBEH BPAEHEM  CAM
              BE. EPO BPAEH PABEH 2.1953D,  1.0256D,
               0.9178D. EPO CA-0.0227D (A=0.01M).
              COACHO  7985! HAATC BA EPOA
              CA: P1=0.0274D  P2=0.0209D (P2/P1=
              =0.76)./MEMBER OF THE COMAE BERENICES CLUSTER.
              LIGHT VARIATIONS ARE DUE TO ROTATION AND PULSATI-
              ONS OF THE STAR. ROTATIONAL PERIOD IS 2.1953D OR
              1.0256D OR 0.9178D. PERIOD OF PULSATIONS IS 0.0227D
              (A=0.01M). ACCORDING TO  7985! THERE ARE TWO PE-
              RIODS OF PULSATIONS: P1=0.0274D AND P2=0.0209D
              (P2/P1=0.76).
UV     COM     FE/H!=-1.44.
UW     COM     FE/H!=-1.22.
UX     COM    MIN II 10.13. P VAR; KBAPATH EH:/NONLINE-
              AR TERM:-3.75D*10**-8*E**2.
UY     COM     FE/H!=-1.51.
UZ     COM     FE/H!=-1.44.
VV     COM     FE/H!=-1.53.
VW     COM    VB (12.00M, DM 3.5E; 12.3M, DM 4E, 3.0", 23G, 1945).
              AH PEE MEHEH CMMAPHOO ECKA.
              COACHO  8363! EPEMEHHM BETC KOMO-
              HEHT B. OHAKO EPEMEHHM MOT T OA
              KOMOHEHTA./RANGE OF TOTAL BRIGHTNESS VARIATION
              IS GIVEN. ACCORDING TO  8363! THE COMPONENT B IS
              VARIABLE. HOWEVER BOTH COMPONENTS MAY BE VARI-
              ABLES.
VY     COM    MIN II 14.5.
AI     COM    EH CKOEH BOOC BEPOHK./MEMBER OF
              THE COMAE BERENICES CLUSTER. VB A (B 6.63M,
              145", 251G). BOMOH CA:/PULSATIONS
              ARE POSSIBLE: P=0.052D (A=0.02M)  8975!.
AL     COM    B 8' K O-BOCTOK OT PA AAKTK M 88
              (NGC 4501)./WITHIN 8' TO THE SOUTH-EAST FROM
              THE NUCLEUS OF M 88 (NGC 4501) GALAXY.
AQ     COM    MIN II 15.7.
BM     COM    MIN II 13.8.
BS     COM    P VAR. MAX=2434453.31+0.36341D*E (J.D.
              2434130-35230); OCE/SINCE J.D.2435590-
              -CM. TA./SEE TABLE. OPMA KPBO ECKA
              MEHETC./SHAPE OF THE LIGHT CURVE VARIES.
BZ     COM     FE/H!=-1.21.
CC     COM    CM./SEE CT COM. MIN II 12.09; DI=0.03P.
CD     COM     FE/H!=-1.78.
CF     COM    OPMA KPBO ECKA MEHETC./SHAPE OF THE
              LIGHT CURVE VARIES.
CG     COM     FE/H!=-1.06.
CI     COM    RRC?
CK     COM    P VAR. MAX=2437370.71+0.6940159D*E (J.D.
              2437370-40130); MAX=2441630.35+0.6939080D*E
              (J.D.2440130-41630); OCE/SINCE J.D.
              2441630-CM. TA./SEE TABLE. EKT A-
              KO/BLAZHKO EFFECT.  FE/H!=-1.68.
CL     COM     FE/H!=-1.00.
CN     COM    MIN II 13.5.
CP     COM     FE/H!=-1.19.
CT     COM    B OACT CKOEH BOOC BEPOHK./IN
              THE REGION OF THE COMAE BERENICES CLUSTER.
CV     COM    CM./SEE CT COM.
CX     COM    CM./SEE CT COM. HE EH CKOEH./NOT
              MEMBER OF THE CLUSTER.
DD     COM    MIN II 14.90.
DG     COM    MIN II 14.6.
DL     COM    P VAR?
DR     COM    EW? P=0.45184D?
DS     COM     FE/H!=-1.32.
DT     COM     FE/H!=-1.60.
DU     COM     FE/H!=-1.45.
DV     COM     FE/H!=-1.57.
DW     COM     FE/H!=-1.53.
EE     COM    P=0.539533D TAKE OBETBOPET HAEH-
              M/ALSO SATISFIES OBSERVATIONS.  FE/H!=-1.64.
EF     COM     FE/H!=-1.90.
EG     COM     FE/H!=-1.29.
EI     COM     FE/H!=-1.68.
EL     COM    P=0.52362D TAKE OBETBOPET HAEHM
              /ALSO SATISFIES OBSERVATIONS.
EM     COM     FE/H!=-1.64.
EN     COM     FE/H!=-1.19.
EO     COM     FE/H!=-1.51.
EP     COM     FE/H!=-0.98.
EQ     COM    MIN II 15.3.
ER     COM     FE/H!=-1.51.
ES     COM     FE/H!=-2.02.
EW     COM     FE/H!=-1.77.
EX     COM    P=0.558359D?  FE/H!=-1.48.
EY     COM    MIN II 18.0.
EZ     COM    P=0.568349D?  FE/H!=-1.16.
FG     COM    P=0.3098D TAKE PECTABET HAEH
              /ALSO SATISFIES OBSERVATIONS.
FK     COM    POKE MCCOHHE H HALFA  H, K CAII
              EPEMEHHO HTEHCBHOCT. AHA OXA MIN
              ECKA./WIDE EMISSION LINES HALFA AND H, K CAII
              OF VARIABLE INTENSITY. EPOCH OF LIGHT MINIMUM IS
              GIVEN.
FM     COM    EH CKOEH BOOC BEPOHK./THE MEMBER
              OF THE COMAE BERENICES CLUSTER. MTEPO-
              HOCT./MULTIPERIODICITY. HAAC TAKE K
              0.0713D  8989!./CYCLE OF 0.0713D WAS OBSERVED
              ALSO  8989!.
FO     COM    CM./SEE CT COM.
FP     COM    CM./SEE CT COM. MU=0.23", P=158G. KPACHA/RED.
FZ     COM    P=4.704864D?
GM     COM    CM./SEE CT COM.
GN     COM    EH CKOEH BOOC BEPOHK./MEMBER OF
              THE COMAE BERENICES CLUSTER. P>1D.
GO     COM    CM./SEE CT COM.
GP     COM    MU=0.38", P=286G. SB (PORB=0.032306D). HKA-
              H O'EKT (G 61-29). COCTOT  BX BA-
              MOECTBX EX KAPKOB, OH 
              KOTOPX (MEHE MACC)-EEB. AB-
              H KOMOHEHT OKPEH AKKPEOHHM CKOM,
              OPAOBAHHM AOBM OTOKOM, TEKM OT
              CTHKA. OHO HAATC BCK C AM-
              TO OKOO 0.2M V, 0.5M U, EC OKOO
              20 CEKH  7417, 8991!. HOA HACTAT E-
              PO OTOMETPECKO AKTBHOCT, KOA
              AMTA MEHEH ECKA OCTAET 0.6M V
               HAATC PEKE EPEXO OT MAKCM-
              MOB K MHMMAM ECKA, EC O 0.14D
               7417!. KOA BEA HAOEE AKTBHA, BOH-
              KAT EPOECKE KOEAH ECKA C P=
              =105 C  AMTO 0.05M-0.10M V  7062!.
              /UNIQUE OBJECT G 61-29. CONSISTS OF TWO INTERAC-
              TING WHITE DWARFS. THE LOWER MASS STAR, A HELIUM
              WHITE DWARF, TRANSFERS MASS TO THE HIGHER MASS
              STAR SURROUNDED BY AN ACCRETION DISK. USUALLY FLA-
              RES ARE BEING OBSERVED WITH AN AMPLITUDE ABOUT
              0.2M V, 0.5M U LASTING ABOUT 20 SECONDS  7417,
              8991!. SOMETIMES PERIODS OF PHOTOMETRIC ACTIVI-
              TY ARISE WHEN AMPLITUDE OF LIGHT VARIATIONS REA-
              CHES 0.6M V AND SHARP PASSAGES FROM MAXIMA TO
              MINIMA ARE BEING OBSERVED; THE DURATION OF THESE
              MINIMA REACHES UP TO 0.14D  7417!. WHEN THE STAR
              IS MOST ACTIVE, PERIODIC LIGHT OSCILLATIONS APPE-
              AR WITH P=105 SECONDS AND AMPLITUDE 0.05M-
              -0.10M V  7062!.
GQ     COM    Z=0.165. MCC/EMISSION H,  OIII!. HEPAB-
              HE MEHEH ECKA/IRREGULAR LIGHT VARIATIONS.
              <B-V>=+0.16.
HH     COM    AHA OXA MIN B CCTEME V./EPOCH OF MIN IN
              V SYSTEM IS GIVEN.
HI_HK  COM    CM./SEE CT COM.
HM_HW  COM    CM./SEE CT COM.
R      CRA    B OOBE PKO KOMETOOPAHO TMAHHOCT
              NGC 6729. K TOK./IN THE HEAD OF THE
              BRIGHT COMETARY NEBULA NGC 6729. IR EXCESS.
S      CRA    VB A (B 13.5M, 1", 137G). K TOK./IR EXCESS.
T      CRA    B PKO KOMETOOPAHO TMAHHOCT NGC 6729.
              K TOK./IN THE BRIGHT COMETARY NEBULA
              NGC 6729. IR EXCESS.
V      CRA    HAAC KBAEPOECKE KOEAH
              (P-75D, DV-0.2M-0.9M). K TOK./QUASIPE-
              RIODIC VARIATIONS (P-75D, DV-0.2M-0.9M). IR
              EXCESS.
RS     CRA    SP  BX KX BE, A  KOTOPX
               OE BMECTE MOT T TOECTBEHH
              COD-39G13082./SP OF TWO CLOSE STARS; EACH OF
              THEM OR BOTH MAY BE IDENTIFIED WITH COD-39G13082.
RW     CRA    MIN II 9.4.
SS     CRA    V1 (NGC 6541).
SV     CRA    BOMOHO, EPO BBOE KOPOE./THE PERIOD
              MAY BE TWICE SHORTER.
TY     CRA    VB A (B 13.3M, 4", 138G; C 58", 24G). B PKO
              TMAHHOCT NGC 6726/27. HE CKEH P=
              =1.92D, TOA MIN II=MIN I. O BAHM HA-
              EHM 8.7-12.4 V (PEOOTEHO "O-
              HA EPEMEHHOCT" -A TPHOCT OEHOK HA
              OHE TMAHHOCT),  BEA KACCPOBA-
              AC KAK INSA./IN THE BRIGHT NEBULA NGC
              6726/27. P=1.92D IS NOT EXCLUDED, IN THAT CASE
              MIN II=MIN I. ON THE BASIS OF VISUAL OBSERVATIONS
              8.7-12.4 V (PRESUMABLY "SPURIOUS VARIABILITY"
              DUE TO THE DIFFICULTIES OF ESTIMATES OVER THE
              BRIGHT BACKGROUND OF THE NEBULA), AND THE STAR
              WAS CLASSIFIED AS INSA.
TZ     CRA    MIN II 9.72.
UU     CRA    MIN II 11.0.
UX     CRA    CM./SEE SV CRA.
UY     CRA    P VAR?
VV     CRA    B PAOHE PKO TMAHHOCT NGC 6729. K -
              TOK./IN THE REGION OF THE BRIGHT NEBULA NGC
              6729. IR EXCESS.
AF     CRA    P VAR. O/BEFORE J.D.2418060 MAX=2413710+
              +483D.*E; OCE/SINCE J.D.2418060-CM. TA.
              /SEE TABLE.
AL     CRA    B-V:+0.65, +1.30.  A/H!=-0.2.
AN     CRA    P VAR. HEHEH EH:/NONLINEAR TERM:
              -0.006D*10**-6*E**2.
AU     CRA    P VAR. HEHEH EH:/NONLINEAR TERM:
              -0.026D*10**-6*E**2.
AY     CRA    MIN II 15.2.
BG     CRA    MIN II 15.1.
BH     CRA    P VAR. HEHEH EH:/NONLINEAR TERM:
              -0.023D*10**-6*E**2.
CM     CRA    P VAR. HEHEH EH:/NONLINEAR TERM:
              -0.007D*10**-6*E**2.
CR     CRA    MIN II 15.7.
CS     CRA    MIN II 15.2.
CY     CRA    P VAR. HEHEH EH:/NONLINEAR TERM:
              -0.002D*10**-6*E**2.
DG     CRA    CM./SEE VV CRA.
DL     CRA    MIN II 13.6.
DN     CRA    P VAR. HEHEH EH:/NONLINEAR TERM:
              +0.006D*10**-6*E**2.
DZ     CRA    D=0.02P.
EE     CRA    <MPG> VAR, 13.5M-15.5M, P2=3000D-5000D
              DM (P1=167D)-1.5M.
EK     CRA    P VAR. O/BEFORE J.D.2422600 MAX=2411870+
              +421D*E.
FF     CRA    O/BEFORE J.D.2423000 MAX=2411530+140.2D*E.
FK     CRA    MIN II 14.5.
FS     CRA    MIN II 14.5.
FW     CRA    O/BEFORE J.D.2416600 MAX=2411190+112.2D*E.
GS     CRA    O/BEFORE J.D.2422600 MAX=2414070+284D*E.
IT     CRA    MIN II 13.6.
KQ     CRA     A/H!=-0.7. B-V:+0.76, +1.23.
KT     CRA    KPACHA./RED.
LU     CRA    P=182D BOMOEH./IS POSSIBLE.
MS     CRA    ETA./YELLOW.
MT     CRA    MIN II 13.1.
NO     CRA    KPACHOBATA./REDDISH.
QR     CRA    KPACHOBATA./REDDISH.
V 347  CRA    B-V:+0.82, +1.17.
V 350  CRA    MIN II 13.4.
V 385  CRA    EPO, BOMOHO, KAC./THE PERIOD
              MAY BE SPURIOUS.
V 413  CRA    (K-B)2=0.11.
V 428  CRA    CM./SEE SV CRA.
V 449  CRA     A/H!=-0.3.
V 454  CRA    MIN II 10.5.
V 455  CRA    D=0.05P. MIN II 13.7.
V 457  CRA    AHA OXA MIN. BOMOEH TAKE T EW,
              TOA P CEET BOT./EPOCH OF MIN IS
              GIVEN. EW TYPE IS ALSO POSSIBLE, IN THAT CASE
              THE VALUE OF P SHOULD BE DOUBLED.
V 465  CRA    MIN II 14.2.
V 467  CRA    P VAR?
V 471  CRA    MIN II 13.3.
V 478  CRA    BPEMEHAM K/SOMETIMES A CYCLE 60D-70D.
V 480  CRA    MIN II 13.9.
V 490  CRA    P VAR? EMEHT PECTABT HAEH
              1944 ./THE ELEMENTS REPRESENT THE OBSERVATI-
              ONS OF 1944.
V 493  CRA    P VAR?
V 501  CRA    MIN II 13.4. BOMOEH OOBHH EPO.
              /TWICE SHORTER PERIOD IS POSSIBLE.
V 503  CRA    D=0.03P.
V 511  CRA    EPO, BOMOHO, HAO BOT./TWICE LON-
              GER PERIOD IS POSSIBLE.
V 512  CRA    P VAR?
V 513  CRA    MIN II 13.2.
V 514  CRA    MIN II 14.0.
V 527  CRA    P VAR.
V 535  CRA    P VAR.
V 541  CRA    P VAR?
V 545  CRA    VB. AH CMMAPH ECK CO CAM CT-
              HKOM./COMBINED BRIGHTNESS WITH A FAINT COM-
              PANION IS GIVEN.
V 553  CRA    P VAR?
V 566  CRA    MIN II 12.7.
V 568  CRA    HOA K/SOMETIMES A CYCLE 60D-80D.
V 569  CRA    MIN II 13.1. BOMOEH T EB./EB TYPE IS
              POSSIBLE.
V 571  CRA    MIN II 14.7.
V 572  CRA    MIN II 14.0.
V 577  CRA    MIN II 13.2. BOMOEH T RR C OOBHHM
              EPOOM./RR TYPE WITH TWICE SHORTER PERIOD
              IS POSSIBLE.
V 578  CRA    BOMOEH T RV C P=118D./RV TYPE WITH
              P=118D IS POSSIBLE.
V 580  CRA    MIN II 14.4.
V 595  CRA    P VAR.
V 601  CRA    AHA OXA MIN./EPOCH OF MIN IS GIVEN.
V 603  CRA    P AE 0.5P EBA AMETH MIN II./SLIGHTLY
              NOTICEABLE MIN II AT THE PHASE 0.5P.
V 604  CRA    D=0.03P.
V 607  CRA    MIN II 14.3.
V 612  CRA    D=0.03P.
V 615  CRA    P VAR?
V 622  CRA    HOA K 55D-60D./SOMETIMES 55D-60D
              CYCLES.
V 633  CRA    P VAR.
V 634  CRA    MIN II 13.9.
V 648  CRA    P AE 0.5P HAMEAETC MIN II./MIN II IS
              FELT AT THE PHASE 0.5P.
V 659  CRA    P=189.4D BOMOEH./IS POSSIBLE.
V 667  CRA    B PAOHE PKO KOMETOOPAHO TMAHHOCT
              NGC 6729. CEKTPAH KACC OEE PAHH,
              EM K./IN THE REGION OF THE BRIGHT COMETARY NE-
              BULA NGC 6729. THE SPECTRAL TYPE IS EARLIER
              THAN K.
V 676  CRA    BOMOEH T RR./RR TYPE IS POSSIBLE.
V 686  CRA    MAX I 5.34, MIN I 5.41, MAX II 5.35, MIN II 5.40
               8970!.
V 691  CRA    4U 1822-37. MCC/EMISSIONS
              CIII/NIII LAMBDA 4640-50, HE II LAMBDA 4686,CIV LAMBDA
1550
               P./ETC.
V 692  CRA    P=0.83D BOMOEH./IS POSSIBLE.
EPSILO CRA    MIN II 4.95.
R      CRB    K TOK./IR EXCESS.
S      CRB    OH, H2O, SIO MAEP/MASER.
T      CRB    VB? A (B<=12M, 0.2"). SB (P=227.6D). CEKTPA-
              H EPO POCEBAETC B OTOMETPEC-
              KX AHHX 1891-1917  1960-1971  8978!.
              OXA EPBO BCK J.D.2402734 (1866). B
               AX HAAC HEOE BCK
              J.D.2438030 (1963)  2442543 (1975)  8979!.
              /THE SPECTRAL PERIOD IS PRESENT IN THE PHOTOMET-
              RIC DATA OF 1891-1917 AND 1960-1971  8978!. THE
              EPOCH OF THE FIRST OUTBURST J.D.2402734 (1866).
              TWO SMALLER OUTBURSTS WERE OBSERVED IN UV LIGHT,
              J.D.2438030 (1963) AND 2442543 (1975)  8979!.
U      CRB    MIN II 7.72. P VAR.
RR     CRB    P2=377D. DM (P1)-0.5M, DM (P2)-0.6M.
RS     CRB    P2=69.5D  1100!. KOEAHE C OCHOBHM EPO-
              OM:/MAIN PERIOD OSCILLATION: 9.1M-11.6M.
RT     CRB    HEHEH EH:/NONLINEAR TERM:
              +2.01D*10**-8*E**2. MIN II 10.52 (VAR). DII=0.09P.
RV     CRB    P VAR. MAX=2428285.608+0.3316217D*E (J.D.
              2428285-31610); MAX=2431705.349+0.3317313D*E
              (J.D.2431705-32954); MAX=2433030.572+
              +0.331705D*E (J.D.2433030-36814)  5496!; MAX=
              =2440001.453+0.331569D*E (1967-1971)  6237!;
              MAX=2441451.413+0.331619D*E (1972-1974)
               7032!. B TAE AH TEKE EMEHT. O
              MEHEHX EPOA CM. TAKE  3506!. EKT
              AKO?/THE TABLE GIVES CURRENT ELEMENTS. ON
              THE PERIOD CHANGES SEE ALSO  3506!. BLAZHKO EFFECT?
RW     CRB    D=0.028P. MIN II 10.29.
TW     CRB    MIN II 11.0.
TZ     CRB    ADS 9979 A (B 6.72M, GIV, 6.6", 233G, 1980).
              SB 2 (P=1.139789D). AHA OXA MIN. HA KAAH-
              HOE B TAE KOEAHE HAKABAETC BTOPOE,
              C TO E AMTO  P=0.1D. AMTA KA-
              AHA  CMMAPHOO ECKA ADS 9979 A  B,
              CPEH BEHA- ADS 9979 A./EPOCH OF
              MIN IS GIVEN. THE VARIATION PRESENTED IN THE TAB-
              LE IS SUPERIMPOSED BY A SECOND ONE, WITH THE SA-
              ME AMPLITUDE AND P=0.1D. THE AMPLITUDE IS GIVEN
              FOR THE COMBINED LIGHT OF ADS 9979 A AND B, THE
              MEAN MAGNITUDE IS FOR ADS 9979 A.
UU     CRB    B HTEPBAE J.D.2444381.73-76 HAAAC
              MEEHHA BCKA C MAKCMAHO AMT-
              O 0.30M B CCTEME IK  0.18M B CCTEME U.
              /DURING J.D.2444381.73-76 A SLOW FLARE WAS OB-
              SERVED, WITH MAXIMAL AMPLITUDE 0.30M IN THE IK
              BAND AND 0.18M IN THE U BAND.
ALFA   CRB    LAMBDA EFF=7230 A: DI=0.034P, DII=0.018P, MIN II-MIN I=
              =0.66P, HA/DEPTH OF MIN I 0.10M, MIN II 0.025M.
BETA   CRB    VB A (B-5M-6M, 0.2", -130G, 1978). SB
              (P=3833.7D). MAHTHOE OE/MAGNETIC FIELD
              VAR, P=18.487D. AHA OXA MIN ECKA./THE
              EPOCH OF MIN LIGHT IS GIVEN.
GAMMA  CRB    ADS 9757 (4.2M, 5.6M; A=0.74", P=91.0A).
U      CRV    VB A (B 13.5M, 0.4' P).
W      CRV    MIN II 11.86. KPBA ECKA ACMMETPHA, PA-
              HOCT BCOT MAKCMMOB 0.10M./THE LIGHT CURVE
              IS ASYMMETRICAL, THE MAXIMA DIFFER IN HIGHT BY
              0.10M.
Y      CRV    MIN II 11.7. BOMOEH T RRC C OOBHHM
              EPOOM./RRC TYPE WITH TWICE SHORTER PERIOD
              IS POSSIBLE.
Z      CRV    D=0.06P.
RV     CRV    MIN II 8.90. EMEHT OBETBOPT HE BCEM
              OKOBAHHM MOMEHTAM MIN./ELEMENTS DO
              NOT SATISFY SOME OF THE PUBLIS HED MOMENTS OF MIN.
RZ     CRV    MIN II 13.9.
SX     CRV    MIN II 9.23. OPMA KPBO ECKA MEHETC. -
              HA MIN I 0.20M, HA MIN II 0.18M. B 1972
              CCTEMA CTAA HA 0.06M CAEE, EM B 1971./THE
              SHAPE OF THE LIGHT CURVE VARIES. DEPTH OF MIN I
              0.20M, DEPTH OF MIN II 0.18M. IN 1972 THE SYSTEM
              BECAME FAINTER THAN IN 1971 BY 0.06M.
R      CRT    PTEHO EPE KAE 2  3 TC
              HE HACTAT EPO OCTOHCTBA ECKA,
              POOAEC O 250D. OH, H2O MAEP./PE-
              RIODS OF LIGHT CONSTANCY WHICH LAST UP TO 250D OC-
              CUR EVERY TWO OR THERE THOUSAND DAYS. OH, H2O
              MASER.
S      CRT    H2O MAEP/MASER.
T      CRT    CPEH ECK/MEAN LIGHT VAR, P2=1006D.
V      CRT    MIN II 10.1; MIN II-MIN I=0.57P.
W      CRT    (K-B)2=+0.21.
X      CRT    (K-B)2=+0.02.
Z      CRT    D=0.016P.
RR     CRT    P=293D /OR 146D BOMOEH/IS POSSIBLE.
RV     CRT    MIN II 9.4:.
SU     CRT     FE/H!>-0.3.
SV     CRT    ADS 8115 A (B 11.5M VIS, 1", 220G). SB 2 (P=
              =5.90513D, ACAHOE BEHE/APSIDAL MOTION,
              P-700A). AHA OXA MIN I B AX B. HA
              MIN II 0.015M. MCC EUII  SRII./EPOCH OF
              MIN I IN B LIGHT IS GIVEN. DEPTH OF MIN II IS 0.015M.
              EUII AND SRII IN EMISSION.
R      CRU    B OACT PACCEHHOO CKOEH/IN THE REGION
              OF THE OPEN CLUSTER NGC 4349.
T      CRU    CM./SEE R CRU.
U      CRU    P VAR. MAX=2410143+351.4D*E (J.D.2410100-
              -14100)  0237!; OCE/SINCE J.D.2437600-CM.
              TA./SEE TABLE.
W      CRU    MIN II 9.3.
SU     CRU     A/H!=-0.8.
SV     CRU    B PAOHE PACCEHHOO CKOEH/IN THE REGION
              OF THE OPEN CLUSTER RUPRECHT 97. HE EH CKOE-
              H/NON-MEMBER OF THE CLUSTER.
SW     CRU    VB A (B 14.0M, 12"). (K-B)2=0.27.
SY     CRU    D=0.05P?
TU     CRU    MIN II 11.5.
TW     CRU    MIN II 12.85:.
TX     CRU    HE CKEHO, TO B ECTBTEHOCT P OPA-
              O KOPOE, HAPMEP, OK K 1D./IT IS NOT EX-
              CLUDED THAT ACTUALLY P IS MUCH SHORTER, CLOSE TO
              1D, FOR INSTANCE.
TZ     CRU    P=2.091140D?
UW     CRU    MIN II 12.9; MIN II-MIN I=0.536P.
UX     CRU    VB A (B 10"). MIN II 12.4; MIN I-MIN II=0.325P;
              DII=0.025P.
VY     CRU    MIN II 13.5.
VZ     CRU    P=1.125810D?
WW     CRU    MIN II 13.0.
WX     CRU    D=0.040P. OTMEEHA EPEMEHHOCT ECKA B
              MAKCMME./LIGHT VARIABILITY IN MAXIMUM IS NO-
              TED.
WY     CRU    VB A. P=9.013290D?
XX     CRU    P=3.28566D?
XY     CRU    MIN II 11.7.
XZ     CRU    P=1.6495930D?
YY     CRU    MIN II 13.0.
YZ     CRU    MIN II 13.1.
ZZ     CRU    MIN II 9.8.
AB     CRU    MIN II 8.9.
AC     CRU    MIN II 12.1.
AD     CRU    VB A (B 14.5M, 10", 270G). P VAR. MAX=2434918.160+
              +6.39844D*E (J.D.2423800-35400)  2309!; OCE
              /SINCE J.D.2441000-CM. TA./SEE TABLE.
AE     CRU    HA/DEPTH OF MIN II 0.03M.
AF     CRU    COACHO  1122!-T EA C EMEHTAM:/ACCOR-
              DING TO  1122! ALGOL-TYPE WITH THE ELEMENTS:
              MIN I=2424988.959+1.895669D*E, D=0.06P. TOT
              BBO TPEET POBEPK. BEA ACBAET
              TATEHOO CCEOBAH./THIS CONCLUSION
              MUST BE CHECKED. THE STAR DESERVES CAREFUL INVE-
              STIGATION.
AG     CRU    BOMOHO HAE OOO CTHKA  9004!.
              /THE BLUE COMPONENT IS POSSIBLE  9004!.
AI     CRU    B OACT PACCEHHOO CKOEH/IN THE REGION
              OF THE OPEN CLUSTER NGC 4103. MIN II 9.94.
AG     CRU    MIN II 13.8.
AT     CRU    MIN II 12.6.
AW     CRU    MIN II 13.9.
AY     CRU    MIN II 11.2.
BB     CRU    MIN II 14.0.
BC     CRU    HA/DEPTH OF MIN II 0.03M.
BD     CRU    HA/DEPTH OF MIN II 0.05M.
BF     CRU    MIN II 12.3.
BH     CRU    AHA OXA MIN I. KPBA ECKA (OOHO KP-
              BM ECKA R CEN  R NOR) MEET BA MAKC-
              MMA  BA MHMMA PAHO H.
              /EPOCH OF MIN I IS GIVEN IN THE TABLE. THE LIGHT
              CURVE LIKE THE LIGHT CURVES OF R CEN AND R NOR
              HAS TWO MAXIMA AND TWO MINIMA OF DIFFERENT
              DEPTHS. MAX I 7.6M (0.22P), MIN II 8.0M (0.41P),
              MAX II 7.2M (0.53P).
BI     CRU    OCAHE CEKTPA/SPECTRUM DESCRIPTION  4949!.
BK     CRU    B OACT OHOO MEKA./IN COALSACK REGION.
BM     CRU    CM./SEE BK CRU.
BP     CRU    3U 1223-62. HKAHA PEHTEHOBCKA CCTE-
              MA. COCTOT  PEHTEHOBCKOO CAPA C E-
              POOM MCOB, PABHM 698S  9018!, B-
              MC O BTHTO OPTE (E=0.47) BOKP
              COAHOO CBEPXAHTA KACCA B2 C
              EPOOM, PABHM 41.51D. AKKPE BEHOO
              BETPA HA CAP CBAETC P POXOE-
              H EO EPE EPACTP, TO PBOT K BOHK-
              HOBEH CHX BCEK PEHTEHOBCKOO -
              EH: T(XMAX)=2433158.09+41.51D*E. BO-
              MOH OTECKE BCK./A UNIQUE X-SYSTEM.
              CONSISTS OF AN X-PULSAR WITH PULSE PERIOD 698S
               9018! MOVING ON AN EXCENTRIC ORBIT (E=0.47)
              AROUND THE ELLIPSOIDAL B2 SUPERGIANT WITH ORBITAL
              PERIOD OF 41.51D. ACCRETION OF THE STELLAR WIND
              FROM THE PRIMARY STAR ON THE PULSAR INCREASES DU-
              RING THE PERIASTRON PASSAGE. THERE FORE LARGE X-
              FLARES ARE OBSERVED WITH THE ELEMENTS: T (XMAX)=
              =2433158.09+41.51D*E. OPTICAL FLARES ARE POSSI-
              BLE.
BQ     CRU    B-V:+1.13, +0.88.
BS_BW  CRU    B PACCEHHOM CKOEH/IN THE OPEN
              CLUSTER NGC 4755.
BETA   CRU    VB A (B 11.4M, 44.3", 322G; C 7.5M, 372", 23G).
              HTEPEPOMETPECKA BOHA/INTERFEROMETRIC
              BINARY. MTEPOHOCT (B CKOKAX KAA-
              H OHE V AMT COOTBETCTBX KO-
              EAH):/MULTIPLE PERIODS (THE TOTAL V AMPLITU-
              DES OF CORRESPONDING OSCILLATIONS ARE INDICATED
              IN BRACKETS): P0=0.2365072D (0.034M), P1=0.160466D
              (0.029M), P2=0.121383D (0.01M), P02=0.249373D
              (0.016M), P13=0.24273D (0.024M), P24=0.23931D
              (0.028M), P03=0.16342D (0.016M), P14=0.16171D
              (0.029M).
TETA** 2      CRU SB (P=3.4380D). BCEPS, P>1H?  8420!.
LAMBDA CRU    BOMOHO, T ELL  P=0.7902D. AMTA 
              OPMA KPBO ECKA MEHTC. BOMOHO
              BTOPOE KOEAHE (A=0.007M) C EMEHTAM
              MAX=2441779.034+0.1793D*E./TYPE ELL WITH
              P=0.7902D IS POSSIBLE. AMPLITUDE AND SHAPE OF
              THE LIGHT CURVE VARY. THE SECONDARY OSCILLATION
              (A=0.007M) WITH THE ELEMENTS MAX=2441779.034+
              +0.1793D*E IS POSSIBLE.
R      CYG    VB A (B 9.3M, 91", 14G). S 4/6E-S 8/6E.
T      CYG    VB A (B 10.03M, 10.2", 122G; C 12M, 13.6", 197G).
U      CYG    VB A (B 7.8M, 63.5", 51G). P VAR. MAX=2406455+
              +461.57D*E (J.D.2404590-13900); MAX=2414827+
              +470.76D*E (J.D.2413900-19940); MAX=2421806+
              +455.95D*E (J.D.2419940-27380); MAX=2427848+
              +472.85D*E (J.D.2427380-35750); OCE/SINCE J.D.
              2435750-CM. TA./SEE TABLE.
W      CYG    HAAETC BTOPOE KOEAHE C P=235.3D./THERE IS
              A SECOND OSCILLATION WITH P=235.3D.
X      CYG    P VAR. MAX=2410190.86+16.3841D*E (J.D.2410100-
              23370)  9028!; OCE/SINCE J.D.2417000-CM. TA./
              SEE TABLE.
              EMEHT, AHHE B TAE, COEPAT KBAPAT-
              H EH: /THERE IS A SQUARE TERM IN THE ELEMENTS GI-
              VEN IN THE TABLE: +1.01D*10**-7*E**2.
               A/H!=0.4.
Y      CYG    MIN II 7.75; E=0.1458. BEHE H AC: /APSI-
              DAL MOTION: P=47.6 YR.
              EMEHT COEPAT CHCOAHE EH: /THERE
              ARE SINUSOIDAL TERMS IN THE ELEMENTS: +0.1391D SIN
              (0.06256G E) -0.0076D SIN 2 (0.06256G E); MIN II =
              =2409454.9174+2.9963328D*E-0.1391D SIN (0.06256G E) -
              -0.0076D SIN 2 (0.06256G E).
Z      CYG    OH, H2O MCC/EMISSION.
RR     CYG    VB A (B 12.5M, 18.1", 58G).
RS     CYG    VB A (B 7.09M, 132", 355G; C 9.3M, 56", 106G). AHA
              OXA MHMMA ECKA. OPMA KPBO ECKA C-
              HO MEHETC. HOA HAATC BOHE MAKCM-
              M (MIN II HA AE 0.5P). /EPOCH OF LIGHT MINIMUM IS
              GIVEN. THE SHAPE OF THE LIGHT CURVE STRONGLY VARIES.
              DOUBLE MAXIMA ARE SOMETIMES OBSERVED (MIN II AT THE
              PHASE 0.5P).
RU     CYG    VB A (B 12.40M V, 10", 224G; C 11.15M V, 19", 29G).
RV     CYG    VB A (B 10M, 142", 118G).
RY     CYG    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF THE
              OPEN CLUSTER NGC 6883.
RZ     CYG    OPMA KPBO ECKA CHO MEHETC. KAK PAB-
              O, HAAETC EPEOBAHE BCOKX  HKX MAK-
              CMMOB, OKX  HEOKX MHMMOB: /THE
              SHAPE OF THE LIGHT CURVE STRONGLY VARIES. ALTERNATION
              OF HIGH AND LOW MAXIMA, AS WELL AS OF SHALLOW AND
              DEEP MINIMA IS OBSERVED, AS A RULE: 9.8M<=MAX<=12.0M.
              11.8M<=MIN<=14.1M.
SS     CYG    SB 2 (P=0.27512995D  8285!). BO BPEM MAKCMMOB
              ECKA HAATC KOEAH ECKA C AMTO
              OKOO 0.002M V  PEHTEHOBCKOO EH C EPO-
              AM, MEHMC B PEEAX 7.29S-10.90S/DU-
              RING MAXIMA OF BRIGHTNESS THERE ARE OSCILLATIONS OF
              LIGHT AND X-RAY FLUX WITH AMPLITUDES ABOUT 0.002M V
              AND PERIODS CHANGING BETWEEN 7.29S AND 10.90S  6102,
              9032!.
SU     CYG    P VAR. MAX=2421278.503+3.845507D*E (J.D.2414250-
              29000)  1559!; MAX=2433095.944+3.845664D*E (J.D.
              2429000-33150)  0921!; OCE/SINCE J.D.2434500-
              CM. TA./SEE TABLE.
SV     CYG    VB A (B 9.5M V, 145", 140G).
SW     CYG    MIN II 9.30; D(V)=0.018P; D(U)=0.00P. P VAR. MIN I =
              =2414782.448+4.572937D*E (J.D.2411340-16450);
              MIN I =2418440.758+4.5727923D*E (J.D.2417060-
              19740)  0063!; MIN I=2421504.489+4.572729D*E (J.D.
              2421470-24970); MIN I =2425185.550+4.5728386D*E
              (J.D.2424960-29500); MIN I =2433160.669+4.5729841D*E
              (J.D.2433000-36800)  9085!; MIN I =2438584.3081+
              +4.57311736D*E (J.D.2438600-40560)  9085!; OCE/
              SINCE J.D.2441160 - CM. TA./SEE TABLE.
SY     CYG    D=0.040P. BOMOHA HA MIN II/POSSIBLE DEPTH
              OF MIN II 0.03M.
              P VAR. MIN I =2411659.568+6.00584D*E (J.D.2411600-
              17100); MIN I =2420001.571+6.005716D*E (J.D.
              2418760-20760)  1961!; MIN I =2437069.254+6.005626D*E
              (J.D.2432800-37070)  5416!.
              B TAE PBEEH CPEHE EMEHT, PECTAB-
              E OX MIN I B HTEPBAE J.D.2414400-
              37070 C TOHOCT O +-0.07D. COACHO  4248!, BO-
              MOHO BPAEHE H AC C EPOOM- 46 ET./
              MEAN ELEMENTS GIVEN IN THE TABLE REPRESENT EPOCHS OF
              MIN I IN THE INTERVAL J.D.2414400-37070 UP TO+-0.07D.
              ACCORDING TO  4248! THE APSIDAL MOTION WITH THE PE-
              RIOD- 46 YEARS IS POSSIBLE.
SZ     CYG     A/H!=0.5. P VAR  2392!. B TAE PBEEH CPE-
              HE EMEHT, PECTABE OX MAX C TO-
              HOCT O +-0.5D. COACHO  9029!, CHCOAH XA-
              PAKTEP APAMM O-C MOET CBETECTBOBAT O
              TOM, TO EPEMEHHA BETC EHOM BOHO C-
              CTEM C P ORB=65 OAM./MEAN ELEMENTS GIVEN IN THE
              TABLE REPRESENT EPOCHS OF MAX UP TO+-0.5D. ACCORDING
              TO  9029! "THE O-C DIAGRAM HAS A SINUSOIDAL STRUC-
              TURE AS IS TO BE EXPECTED FOR A MEMBER OF A BINARY SY-
              STEM" WITH P ORB=65 YEARS.
TT     CYG    VB A (B 10.8M V, 70", 213G; C 11.1M V, 83", 49G;
              D 10.7M V, 94", 268G).
TV     CYG    COACHO/ACCORDING TO  3663! -CEKTP/SPECTRUM GO.
TX     CYG     A/H!=-0.2. P VAR. MAX=2436793.138+14.708157D*E
              (J.D.2415000-37000); OCE/SINCE J.D.2436700-
              CM. TA./SEE TABLE.
UU     CYG    VB A (B 10.7M V, 3.6", 351G).
UV     CYG    VB A (B 10.8M V, 0.9", 79G).
UW     CYG    P VAR. MIN I =2419624.501+3.450797D*E (J.D.2410000-
              20750)  0526!; MIN I =2419624.501+3.450752D*E (J.D.
              2419620-33000); MIN I =2433848.508+3.450740D*E
              (J.D.2430000-41800); OCE/SINCE J.D.2441800-CM.
              TA./SEE TABLE. BOMOHA HA MIN II/POS-
              SIBLE DEPTH OF MIN II 0.05M.
UX     CYG    P VAR. MAX=2432444+560.3D*E (J.D.2415670-32450);
              MAX=2439352+578.0D*E (J.D.2432450-40500); OCE/
              SINCE J.D.2437600-CM. TA./SEE TABLE.
              HOA HAATC CTPE OCAEH ECKA HA
              BOCXOE BETB  MAX/SOMETIMES RAPID LIGHT DEC-
              REASES ON THE ASCENDING BRANCH NEAR MAX ARE OBSERVED
               1563, 1564!. H2O, OH, SIO MAEP/MASER.
UY     CYG    DS=3.8.
UZ     CYG    VB A (B 10.8M, 28", 130G). D=0.032P; MIN II 10.31.
VV     CYG    MIN II 13.2. P VAR?  3665!.
VW     CYG    D=0.035P; MIN II 10.31. P VAR. MIN I =2417377.123+
              +8.4305260D*E (J.D.2415660-17400); MIN I =
              =2430444.061+8.4302826D*E (J.D.2417400-30450);
              MIN I =2441116.868+8.4303917D*E+4.31D*10**-8*E**2 (J.D.
              2430450-41120)  7096!; OCE/SINCE J.D.2440350-
              CM. TA./SEE TABLE.
              -0.000107D*10**-6*E**2 (J.D.2414000-35000)  2550!;
              MAX=2438562.796+0.466570D*E (J.D.2434000-39800);
              MAX=2440445.789+0.466497D*E (J.D.2439800-41000)
               6237!; MAX=2441453.3856+0.4664731D*E (J.D.
              2441000-42500)  7424!; MAX=2443028.641+
              +0.466438D*E (J.D.2442500-43800)  9101!; MAX=
              =2444142.650+0.466649D*E (J.D.2443800-44200)
               9102!; OCE/SINCE J.D.2444100-CM. TA./SEE
              TABLE.
              KPOME TOO, BEA OAAET PEKO BPAEHHM -
              EKTOM AKO, EPO KOTOPOO TAKE MEHETC
               7424, 7425!./BESIDES THAT THE STAR HAS A STRONGLY
              EXPRESSED BLAZHKO EFFECT; THE PERIOD OF BLAZHKO EF-
              FECT VARIES, TOO  7424, 7425!. 0.13P<=M-M<=0.22P; 0.90M<=
              <=A(B)<=1.70M, 0.70M<=A(B)<=1.30M; -0.05P<O-C<+0.05P;
              MAX A =2417025.5+57.401D*E (J.D.2417000-38500);
              MAX A =2438881.7+58.387D*E (OCE/SINCE J.D.
              2438500).!9103!.
              OCE J.D.2444000, BOMOHO, EPO EKTA A-
              KO MEHC O 56.3D  9102!./AFTER J.D.2444000
              BLAZHKO EFFECT PERIOD PROBABLY DECREASED TO 56.3D  9102!.
ZZ     CYG    VB A (B 12.63M, 8.5", 43G). AH PEE MEHEH
              CMMAPHOO ECKA./TOTAL BRIGHTNESS VARIATION RANGE
              IS GIVEN. MIN II 10.78. P VAR. MIN I =2417442.419+
              +0.6286185D*E (J.D.2415000-25800)  7427!; OCE/
              SINCE J.D.2427950 - CM. TA./SEE TABLE.
AA     CYG    S 6/3.
AC     CYG    H2O MAEP/MASER.
AD     CYG    S 5/5.
AE     CYG    D=0.039P; HA/DEPTH OF MIN II 0.06M.
AF     CYG    KPBA ECKA/LIGHT CURVE (1914-1956909104!. HA-
              AETC HAOEHE EE BX HEABCMX KOE-
              AH:/TWO MORE INDEPENDENT OSCILLATIONS ARE SUPER-
              IMPOSED: P2=175.8D, P3=941.2D.
AK     CYG    VB A (B 11.06M, A7, 20", 85G).
AV     CYG    P VAR. MAX=2420451.9+87.48D*E (J.D.2418782-
              24823); MAX=2427936.3+89.73D*E (J.D.2426326-
              28745); MAX=2429440.9+87.69D*E (J.D.2428820-
              31260); MAX=2436413.8+89.63D*E (J.D.2434610-
              37130); OCE/SINCE J.D.2437450 - CM. TA./SEE
              TABLE. 0.27P<=M-M<=0.50P.
AX     CYG    VB A (B 10.2M, 18", 52G).
AY     CYG    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF THE
              OPEN SLUSTER DOLIDZE 2.
BB     CYG    P VAR. MAX=2426360+265.7D*E (J.D.2414900-26700);
              MAX=2433091+258.6D*E (J.D.2426700-35500); MAX=
              =2438354+266.9D*E (J.D.35500-40200)  9106!; O-
              CE/SINCE J.D.2439200 - CM. TA./SEE TABLE.
BF     CYG    P ORB =750D  5655!. HA HEPABHE MEHEH EC-
              KA  HAAEME HOA OPAH HA 2-3M HAKA-
              BATC OPABHE KOEAH C KOM 755D/
              IRREGULAR LIGHT VARIATIONS AND SOMETIMES OBSERVED
              BRIGHTENINGS BY 2M-3M ARE SUPERIMPOSED BY SEMIRE-
              GULAR OSCILLATIONS WITH THE CYCLE 755D  1039, 8044!.
BG     CYG    P VAR. MAX=2421190+290.35D*E (J.D.2421150-29950);
              MAX=2430546+307.3D*E (J.D.2429950-30850); MAX=
              =2432872+289.5D*E (J.D.2430850-34920); OCE/
              SINCE J.D.2435100-CM. TA./SEE TABLE.
BI     CYG    VB A (B 9.4M, 126", 110G).
BO     CYG    D=0.025P; MIN II 12.0.
BR     CYG    D=0.020P; MIN II 9.58.
BS     CYG    SC 8/8. P VAR. MAX=2422655+420D*E (J.D.2422600-
              24750)  1161!; MAX=2425181+431.4D*E (J.D.2424750-
              26500)  1171!; OCE/SINCE J.D.2437500-CM. TA./
              SEE TABLE.
BY     CYG    VB A (B 16M).
BZ     CYG     A/H!=0.1. MAKCMM - BOHO./DOUBLE MAXIMUM.
CD     CYG     A/H!=0.2. P VAR. EMEHT COEPAT KBAPAT-
              H EH:/THERE IS A SQUARE TERM IN THE ELEMENTS:
              +1.54D*10**-6*E**2.
CG     CYG    VB A (B 11.8M, 1.3", 306G; 1979.7). 10.10<=MIN II<=10.44.
              P VAR. MIN I =2422967.4248+0.63114347D*E (J.D.
              2422900-38500); OCE/SINCE J.D.2439000-CM. TA./
              SEE TABLE.
              AH PEE MEHEH CMMAPHOO ECKA. OPMA
              KPBO ECKA MEHETC  8848!./COMBINED LIGHT RANGE
              IS GIVEN. SHAPE OF THE LIGHT CURVE VARIES  8848!.
CH     CYG    OPABHE KOEAH ECKA CO CPEHM K-
              OM 97D; CPEH ECK MEHETC C KOM-4700D
               1169!. HAAETC TAKE K 725D  8849!, CT-
              PA EPEMEHHOCT (A<=0.25M U)  BCK  5350!. HE
              CKEHO, TO CCTEMA BETC ATMEHHO  6499!./
              SEMIREGULAR LIGHT VARIATIONS WITH THE MEAN CYCLE 97D;
              MEAN BRIGHTNESS VARIES WITH THE CYCLE-4700D  1169!.
              THERE ARE ALSO A CYCLE 725D  8849!, RAPID OSCILLA-
              TIONS (A<=0.25M U) AND FLARES  5350!. IT IS NOT EXCLUDED
              THAT THE SYSTEM IS AN ECLIPSING ONE  6499!.
CI     CYG    D=0.084P. HA ATMEH-0.8M. HAATC A-
              TMEH B-BE. OHO KTA OKOO CPE-
              HEO ECKA (-12.1M). BCK POOATC E-
              CTK  COTH HE. KPBE ECKA  6155, 8044,
              8850, 8851!. MCC H, HE I, HE II,  O III!, N III./
              DEPTH OF ECLIPSES-0.8M. THE ECLIPSES OF B STAR ARE OBSER-
              VED. USUALLY THERE ARE LIGHT FLUCTUATIONS NEAR MEAN
              BRIGHTNESS (-12.1M). THE OUTBURSTS LAST SOME DOZENS
              AND HUNDREDS DAYS. LIGHT CURVES  6155, 8044, 8850,
              8851!. EMISSIONS OF H, HE I, HE II,  O III!, AND N III.
CM     CYG    S 4/6.5E.
CU     CYG    P VAR. MAX=2422643+223.8D*E (J.D.2422600-26500);
              OCE/SINCE J.D.2426500-CM. TA./SEE TABLE.
CV     CYG    D I =0.06P; MIN II 11.33. P VAR. MIN I =2424458.348+
              +0.9834523D*E (J.D.2414300-24500); OCE/SINCE J.D.
              2424450-CM. TA./SEE TABLE.
              OPMA KPBO ECKA  HA MIN I MEHTC./
              SHAPE OF THE LIGHT CURVE AND MIN I DEPTH VARY.
CY     CYG    SC 2/7.5.
CZ     CYG    P VAR. MAX=2424500+284D*E (J.D.2424500-33600)
               3122!; OCE/SINCE J.D.2432700-CM. TA./SEE
              TABLE.
DD     CYG    P VAR. MAX=2425465+148.30D*E (J.D.2424800-39000)
               1149!; OCE/SINCE J.D.2439000-CM. TA./SEE
              TABLE.
DF     CYG    P VAR  1177, 6107!. CPEH ECK MEHETC:/MEAN
              BRIGHTNESS VARIES: MIN=2411292+780.2D*E  1571!.
DG     CYG    SIO MAEP?/MASER?
DH     CYG    OH MCC?/EMISSION?
DK     CYG    D I = D II =0.04P; MIN II 10.90. P VAR. OPMA KPBO
              ECKA  HA MIN II MEHTC./SHAPE OF THE
              LIGHT CURVE AND DEPTH OF MIN II VARY.
DL     CYG    MIN II 9.9.
DM     CYG    P VAR. MAX=2425887.560+0.4198557D*E (J.D.2415200-
              25900)  3506!; MAX=2425887.5597+0.41985715D*E
              (J.D.2425880-29250)  0522!; MAX=2433872.420+
              +0.41985842D*E (J.D.2429250-37900)  3506!; MAX=
              =2438677.708+0.4198619D*E (J.D.2438600-41250)
               7114!; OCE/SINCE J.D.2441240-CM. TA./SEE
              TABLE.
              KPOME TOO, HAAETC EKT AKO C EMEH-
              TAM:/THERE IS ALSO BLAZHKO EFFECT WITH THE ELEMENTS:
              MAX(O-C)=2442978.97+26.01D*E  8853!; -0.01D<=
              <=O-C<=+0.01D. DS=0.
DQ     CYG    P=180D?
DT     CYG    P VAR. MAX=2424305.651+2.49913D*E (J.D.2424300-
              28500)  1183!; MAX=2432792.893+2.49934D*E (J.D.
              2430000-36000); OCE/SINCE J.D.2436000-CM. TA./
              SEE TABLE.
DV     CYG    P VAR. MAX=2425476+146.7D*E (J.D.2415200-29200);
              OCE/SINCE J.D.2432800-CM. TA./SEE TABLE.
DW     CYG    P VAR. MAX=2427603+279.6D*E (J.D.2416700-33500);
              OCE/SINCE J.D.2433500-CM. TA./SEE TABLE.
DX     CYG    MIN II 14.2; MIN II - MIN I =0.515P; DI=0.22P, DII=0.12P.
DY     CYG    HA MEEHHE KOEAH HAKABATC CTPE C
              A=0.3M  3662!. COACHO  3148!, T EB?/SLOW OSCIL-
              LATIONS ARE SUPERIMPOSED BY RAPID ONES WITH A=0.3M
               3662!. ACCORDING TO  3148! TYPE EB? MIN=2436659.531+
              +0.6990D(:)*E (J.D.2436600-37000)  3148!.
EE     CYG    MIN II 14.5.
EF     CYG    142D<=P<=175D.
EH     CYG    P VAR. MAX=2427608+276.90D*E (J.D.2416200-27610);
              OCE/SINCE J.D.2427800-CM. TA./SEE TABLE.
EI     CYG    AHA OXA MAX I; BCOT MAX I  MAX II CHO PA-
              ATC, H MIN I  MIN II OT OHAKOB./
              EPOCH OF MAX I IS GIVEN; HEIGHTS OF MAX I AND MAX II
              DIFFER STRONGLY, THE DEPTHS OF MIN I AND MIN II ARE ALMOST
              EQUAL. MAX I - MIN I =52D.
EK     CYG    EMEHT PECTABT HAEH TOKO B HTEP-
              BAE J.D.2425200-37900./OBSERVATIONS ARE REPRE-
              SENTED BY THE ELEMENTS IN THE INTERVAL J.D.2425200-
              37900 ONLY.
EM     CYG    CPEH K MEHETC B PEEAX 19D-33D  4248,
              9111!. HA ATMEH 0.25M V; EMEHT MEHE-
              H ECKA ATMEHHO CCTEM: MIN=2437882.8595+
              +0.29090950D*E-21.10D**-12*E**2  8854!. HOA OC-
               ECKA C EPOAM 14.6S-21.2S  AMTO
              O 0.4%  6102, 9112!./MEAN CYCLE VARIES IN THE RANGE
              19D-33D  4248, 9111!. DEPTH OF ECLIPSES 0.25M V; ELE-
              MENTS OF ECLIPSING SYSTEM LIGHT VARIATIONS: MIN =
              =2437882.8595+0.29090950D*E-21D*10**-12*E**2  8854!.
              SOMETIMES THERE ARE LIGHT OSCILLATIONS WITH PERIODS
              14.6S-21.2S AND AN AMPLITUDE UP TO 0.4%  6102, 9112!.
EN     CYG    D=0.012P. P VAR. MIN=2425181.311+2.2148998D*E
              (J.D.2424880-29600)  0332!; OCE/SINCE J.D.2433500-
              CM. TA./SEE TABLE.
ES     CYG    P VAR. MAX=2425146+157D*E (J.D.2425000-29300)
               0332!; OCE/SINCE J.D.2432800-CM. TA./SEE
              TABLE.
EV     CYG    P VAR. MAX=2427740+259.1D*E (J.D.2425100-29100);
              OCE/SINCE J.D.2433500-CM. TA./SEE TABLE.
              OOEHE BE HA KAPTE B  0530! KAAHO HEBEP-
              HO  0782!./THE POSITION OF THE STAR IN THE CHART IN
               0530! IS WRONG  0782!.
EZ     CYG    P VAR? OPMA KPBO ECKA  AMTA CHO ME-
              HTC; /SHAPE OF THE LIGHT CURVE AND THE AMPLITUDE
              STRONGLY VARY; 0.40P<=M-M<=0.48P.
FF     CYG    S 5.5/6-E.
FG     CYG    P VAR. MAX=2426955+456.0D*E (J.D.2416000-27000)
               0001!; MAX=2426955+458.8D*E (J.D.2426900-34300)
               3122!; OCE/SINCE J.D.2439200-CM. TA./SEE
              TABLE.
FM     CYG    P VAR. MAX=2425313+274D*E (J.D.2425300-29200)
               0332!; OCE/SINCE J.D.2429200-CM. TA./SEE
              TABLE.
FN     CYG    P VAR. MAX=2429137+314.6D*E (J.D.2416200-29200)
               0001!; OCE/SINCE J.D.2432800-CM. TA./SEE
              TABLE.
FO     CYG    A VAR. P VAR. MAX=2425193+156.6D*E (J.D.2425000-
              29200)  0332!; OCE/SINCE J.D.2432500-CM. TA./
              SEE TABLE.
FR     CYG    MIN II 14.0; D=0.03P.
FT     CYG    P VAR. MAX=2425184+156.7D*E (J.D.2425100-29200)
               0332!. 83D<=P<=187D (J.D.2432500-38000).
FY     CYG    P VAR. MAX=2425172+194.D*E (J.D.2425100-29300)
               0332!. 130D<=P<=189D (J.D.2432500-38000).
GG     CYG    D=0.079P; MIN II 12.1.
GM     CYG    P VAR. MIN=2428754.305+4.745772D*E (J.D.2413200-
              33500)  1209!; OCE/SINCE J.D.2433500-CM. TA./
              SEE TABLE.
GN     CYG    P VAR. MAX=2425448+156D*E (J.D.2425400-27400)
               1155!; OCE/SINCE J.D.2427500-CM. TA./SEE
              TABLE.
GO     CYG    MIN II 8.73. P VAR. BOMOHA ECKA EPEMEH-
              HOCT ECKA KOMOHEHTOB/INTRINSIC LIGHT VARIABILITY
              OF THE COMPONENTS IS POSSIBLE  1210!.
GS     CYG    P=195D?
GT     CYG    HA/DEPTH OF MIN II 0.05M? P VAR?
GY     CYG    BOMOHO BTOPHOE KOEAHE C P=4000D  A(V)=
              =0.5M./SECONDARY OSCILLATION WITH P=4000D AND A(V)=
              =0.5M IS POSSIBLE.
GZ     CYG    KPACHA/RED.
HL     CYG    D=0.02P.
HV     CYG    VB (CEBEPH KOMOHEHT/NORTHERN COMPONENT).
HY     CYG    P VAR. MAX=2425334+344D*E (J.D.2425300-29200)
               0332!; OCE/SINCE J.D.2432760-LB?
II     CYG    P VAR. MAX=2425150+82D*E (J.D.2425120-25550),
              MAX=2425475+94D*E (J.D.2425550-29250)  0332!;
              OCE/SINCE J.D.2432500 77D<=P<=99D.
IK     CYG    P VAR. MAX=2425199+77.3D*E (J.D.2425000-29200)
               0332!; OCE/SINCE J.D.2432500-CM. TA./SEE
              TABLE.
IT     CYG    P VAR. MAX=2425305+67.4D*E (J.D.2425300-850)
               0332!; OCE/SINCE J.D.2432500-CM. TA./SEE TABLE.
IU     CYG    B-V:+0.90, +1.45. P VAR. MAX=2429157.6+31.22266D*E
              (J.D.2417800-29250); MAX=2433601.3+31.1550D*E
              (J.D.2432700-35400); OCE/SINCE J.D.2435400-CM.
              TA./SEE TABLE.
IV     CYG    P VAR. MAX=2425470.406+0.33432871D*E (J.D.2425300-
              33120)  3506!; MAX=2434122.519+0.33433895D*E (J.D.
              2432700-40200)  4248!; OCE/SINCE J.D.2440200-CM.
              TA./SEE TABLE.
              OPMA KPBO ECKA MEHETC:/SHAPE OF THE LIGHT
              CURVE VARIES: 0.10P<=M-M<=0.20P.
IX     CYG    P VAR. MAX=2425173+172D*E (J.D.2425000-25900)
               0332!; OCE/SINCE J.D.2428000-CM. TA./SEE
              TABLE.
KL     CYG    P VAR. MAX=2437906+536.8D*E (J.D.2418500-38000)
               0001!; OCE/SINCE J.D.2438000-CM. TA./SEE
              TABLE.
KP     CYG    DS=0.
KR     CYG    MIN II 9.37.
KU     CYG    MIN II 11.15; D=0.047P. OPMA KPBO ECKA MEHET-
              C/SHAPE OF THE LIGHT CURVE VARIES.
KV     CYG    MIN II 11.9.
KY     CYG    H2O, OH MAEP/MASER.
LN     CYG    MIN II 14.3.
LO     CYG    MIN II 13.3.
LX     CYG    P VAR. MAX=2432775+460.0D*E (J.D.2415000-33300)
               1159!; OCE/SINCE J.D.2437900-CM. TA./SEE
              TABLE. SC 7/9-E - SC 8/8.5E.
MQ     CYG    VB A (B 17.5M B, 4.5", 122G). P VAR. MAX=2432737+
              +428.5D*E (J.D.2414300-33300)  1229!; OCE/SINCE
              J.D.2440000-CM. TA./SEE TABLE.
MR     CYG    MIN II 9.12; D=0.030P; DII=0.19P.
MU     CYG    MIN II 14.4.
MY     CYG    MIN II 8.99. MIN II - MIN I =0.5021P.
MZ     CYG    P VAR. MAX=2427641.914+21.162460D*E+0.10575D*
              *10**-3*E**2 (J.D.2414900-37900)  3689!; OCE/SINCE
              J.D.2443600-CM. TA./SEE TABLE.
              BOMOHO, OTHOCTC K T RV TAU,  B TAKOM C-
              AE EPO CEET BOT  8862!./PROBABLY IT IS
              AN RV TAU TYPE VARIABLE, AND THEN THE PERIOD SHOULD
              BE DOUBLED  8862!.  A/H!=0.1.
NQ     CYG    BOMOEH T EW. HEAEKO OT V736 CYG./EW TYPE
              IS POSSIBLE. CLOSE TO V736 CYG.
NU     CYG    MIN II 14.9.
NZ     CYG    MIN II 14.2.
OS     CYG    P VAR.
OU     CYG    MIN II 15.6.
OY     CYG    BEA/STAR 23-30  1321!.
PP     CYG    BEA G HA KAPTE  VV245  7749!./STAR G IN THE
              CHART FOR VV245  7749!.
PR     CYG    BEA/STAR 24-40  1321!.
PT     CYG    BEA/STAR 23-55  1321!.
PU     CYG    BEA/STAR 25-56  1321!.
PX     CYG    BEA/STAR 35-78  1321!.
PY     CYG    MIN II 15.2.
QS     CYG    MIN II 13.3.
QT     CYG    HA MIN II/DEPTH OF MIN II 0.04M.
QU     CYG    MIN II 15.1.
QW     CYG    MIN II 14.1.
QX     CYG    MIN II 14.5.
V339   CYG    NP KOMOHEHT TECHO BOHO./NP COMPONENT OF A
              CLOSE BINARY.
V340   CYG    MIN II 14.5.
V343   CYG     A/H!=-0.2.
V346   CYG    CTHK/COMPANION 13.8M, 0.4' SF. MIN II 11.9. P VAR.
              MIN I =2427270.241+2.743345D*E (J.D.2415000-32000);
              OCE/SINCE J.D.2432000-CM. TA./SEE TABLE.
V348   CYG    COACHO  7516! EPEMEHHOCT TA EW C OM
              HEPABHOCTM:/ACCORDING TO  7516! EW TYPE VA-
              RIABLE WITH LARGE IRREGULARITIES: MIN=2441567.177+
              +0.285768D*E (J.D.2441567-95).
V355   CYG    MIN II 14.3.
V360   CYG    P VAR  6107!. MIN I =2429187.4+70.449D*E (J.D.
              2414600-34000)  0580!; OCE/SINCE J.D.2426000-CM.
              TA./SEE TABLE.
V366   CYG    MIN II 10.2.
V367   CYG    VB A (A 0.1", 50G; B 13.7M, 2.3", 255G). MIN II 7.16. OP-
              MA KPBO ECKA  EBX CKOPOCTE MEHETC./
              SHAPE OF THE LIGHT CURVE AND THE RADIAL VELOCITY CURVE
              VARY.
V368   CYG    COACHO  0204!, T EB (12.8M-13.8M PG) C EMEH-
              TAM:/ACCORDING TO  0204! EB TYPE (12.8M-13.8M PG)
              WITH THE ELEMENTS: MIN I =2425808.10+0.47586D*E
              (J.D.2425805-853).
V369   CYG    P VAR. MAX=2438199+104.46D*E (J.D.2426000-38200);
              OCE/SINCE J.D.2438200-CM. TA./SEE TABLE.
V370   CYG    MIN II 11.9. P VAR. MIN I =2425096.429+0.77453979D*E
              (J.D.2414400-30000); OCE/SINCE J.D.2430000-CM.
              TA./SEE TABLE.
V371   CYG    MIN II 12.5.
V374   CYG    D=0.03P.
V380   CYG    MIN II 5.76; MIN II - MIN I =0.418P (1963). EMEHT CO-
              EPAT OOHTEHE EH:/THERE ARE PERIODIC
              TERMS IN THE ELEMENTS: +0.8916D SIN (38.8G+0.0082G*E)-
              -0.0796D SIN (77.6G+0.0164G*E)+0.0088D COS (26.4G+
              +0.0246G*E);  MIN II =2441262.266+12.425612D*E-
              -0.8916D SIN (38.8G+0.0082G*E)-0.0796D SIN (77.6G+
              +0.164G*E)-0.0088D COS (26.4G+0.0246G*E).
              BOMOHO BEHE H AC C P=1490 ET./
              APSIDAL MOTION IS POSSIBLE WITH P=1490 YEARS.
V382   CYG    VB A (B 11.5M, 11", 332G). MIN II 9.12. OPMA KPBO
              ECKA  HA MIN II MEHTC./SHAPE OF THE
              LIGHT CURVE AND DEPTH OF MIN II VARY. P VAR. MIN I =
              =2427992.458+1.885497D*E (J.D.2413480-29500)
               1253!; OCE/SINCE J.D.2428000-CM. TA./SEE
              TABLE.
V385   CYG    MIN II 12.4.
V387   CYG    MIN II 11.6.
V388   CYG    MIN II 9.15; D=0.06P. P VAR. MIN I =2433584.540+
              +0.8590507D*E (J.D.2427600-37200); OCE/SINCE
              J.D.2437200-CM. TA./SEE TABLE.
V389   CYG    VB A (B 8.0M, 3.4", 305G, 1980). SB (P=3.313168D); O-
              PAAETC BOKP HEBMOO TPETEO CTHKA C
              P=154.09D./TURNS AROUND THE INVISIBLE THIRD COMPA-
              NION WITH P=154.09D.
              COACHO  1256!, MEHEH ECKA POCXOT C
              BM EPEMC EPOAM P1  P2. EPBOE
              KOEAHE (P1) C A=0.19M OBETBOPET EMEH-
              TAM: MAX=2423298.460+1.12912D*E, BTOPOE (P2) C
              A=0.05M-EMEHTAM: MAX=2429162.080+1.19328D*E.
              KAOE  HX POOAETC B TEEHE 1-3 HEE.
              P EPEXOE OT OHOO K POM HOA HAA-
              TC HEPABHE MEHEH ECKA  OT O-
              CTOHCTBO EO. P BOOHOBEH KAOO KOEA-
              H AA EO COXPAHETC, HE CTBA CKAKA.
              COACHO  8909!, B 1975-1977 EPOHOCT HE HA-
              AAC./ACCORDING TO  1256! THE LIGHT VARIES WITH
              TWO ALTERNATE PERIODS P1 AND P2. THE FIRST OSCILLATION
              (P1) WITH A=0.19M SATISFIES THE ELEMENTS: MAX=
              =2423298.460+1.12912D*E, THE SECOND (P2) WITH A=
              =0.05M-THE ELEMENTS: MAX=2429162.080+1.19328D*E.
              EACH OF THEM CONTINUES FOR 1-3 WEEKS. AT THE TRANSI-
              TION FROM ONE OSCILLATION TO THE OTHER IRREGULAR LIGHT
              VARIATIONS ARE SOMETIMES OBSERVED OR ALMOST CONSTANT
              BRIGHTNESS. AT THE RENEWAL OF EACH OSCILLATION ITS PHASE
              REMAINS UNCHANGED, EXPERIENCING NO SHIFT. ACCORDING
              TO  8909! IN 1975-1977 PERIODICITY WAS NOT OBSERVED.
V393   CYG    D=0.02P.
V401   CYG    MIN II 11.13. P VAR. MIN I =2432881.277+0.582717D*E
              (J.D.2428800-34000); OCE/SINCE J.D.2434000-CM.
              TA./SEE TABLE.
V402   CYG    VB A (B 20", 90G).
V407   CYG    VB A (B 14.0M, 8", 190G).  HA KOEAH ECKA EPE-
              MEHHO TA MP KTA HAOEHA BCKA, O-B-
              MOM, HOBO, POCEA OKOO J.D.2428400 (1936)
              C OCEM MEEHHM AEHEM ECKA. CEKTP
              KOMHPOBAHH./LIGHT VARIATIONS OF THE MIRA TYPE
              VARIABLE ARE SUPERIMPOSED BY THE OUTBURST OF THE PRO-
              BABLE NOVA WHICH OCCURED NEAR J.D.2428400 (1936)
              WITH THE CONSEQUENT SLOW LIGHT DECREASE. COMBINED
              SPECTRUM.
V411   CYG    P VAR. MAX=2421075+321D*E (J.D.2421000-31100)
               1262!; OCE/SINCE J.D.2431100-CM. TA./SEE
              TABLE.
V416   CYG    KPACHA/RED.
V425   CYG    OCAHE CEKTPA  EO MEHEH  2685, 3149!./DES-
              CRIPTION OF THE SPECTRUM AND ITS VARIATIONS  2685, 3149!.
V427   CYG    P VAR. MAX=2425471+143D*E (J.D.2425400-5950)
               1155!; OCE/SINCE J.D.2433850-CM. TA./SEE
              TABLE.
V429   CYG    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF THE
              OPEN CLUSTER NGC 6883.
V430   CYG    CM./SEE V429 CYG. MAX=2425544+258D*E (J.D.
              2425500-27400)  1155!.
V432   CYG    B PAOHE PACCEHHOO CKOEH OE 3./IN THE
              REGION OF THE OPEN CLUSTER DOLIDZE 3.
V439   CYG    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER BERKELEY 87= OCL 161.
V441   CYG    AHA OXA MIN I/EPOCH OF MIN I IS GIVEN.
V442   CYG    MIN II 10.4:, D=0.01P:. COACHO  8721!, EPO, AH-
              H B  0525!, OEH T BOEH./ACCORDING TO
               8721! THE PERIOD GIVEN IN  0525! MUST BE DOUBLED.
V443   CYG    D=0.04P. EMEHT COEPAT EPOECK EH:/
              THERE IS A PERIODIC TERM IN THE ELEMENTS:
              -0.016D SMN 0.00105*E.
V444   CYG    B OACT H II/IN THE H II REGION S 109. MIN II 8.06;
              D II =0.10P. P VAR. MIN I =2430856.453+4.21238D*E (J.D.
              2415000-30000)  0007!; OCE/SINCE J.D.2430000-CM.
              TA./SEE TABLE.
V445   CYG    P VAR. MIN=2425527.391+1.947833D*E (J.D.2425500-
              34700)  1155!; OCE/SINCE J.D.2434700-CM. TA./
              SEE TABLE.
V447   CYG    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF THE
              OPEN CLUSTER NGC 6871.
V448   CYG    CM./SEE V447 CYG. MIN II 8.40.
V450   CYG    KPBA ECKA OXOA HA KPB ECKA DQ HER./THE
              LIGHT CURVE RESEMBLES THAT OF DQ HER.
V453   CYG    CM./SEE V447 CYG. MIN II 8.68; D=0.03P; MIN II - MIN I =
              =0.5077P. COACHO  7518! HAAETC BEHE -
              H AC C P=71 O./ACCORDING TO  7518! THERE IS
              APSIDAL MOTION WITH P=71 YEARS.
V454   CYG    MIN II 12.3. B PAOHE PACCEHHOO CKOEH/IN THE
              REGION OF THE OPEN CLUSTER IC 4996.
V455   CYG    MIN II 10.9. P VAR. MIN I =2431151.908+8.7689331D*E
              (J.D.2426800-33950)  1286!; OCE/SINCE J.D.2436800-
              CM. TA./SEE TABLE.
V456   CYG    MIN II 11.4; MIN II - MIN I =0.518P. P VAR?
V457   CYG    MIN II 13.9.
V458   CYG    MIN II 14.2.
V461   CYG    PB=7000D?  8251!.
V462   CYG    P VAR. MAX=2428540+376.0D*E (J.D.2416000-35200);
              OCE/SINCE J.D.2435200-CM. TA./SEE TABLE.
V463   CYG    MIN II 10.65; MIN II - MIN I =0.514P.
V465   CYG    MEETC TECH CTHK 17.5M./THERE IS A CLOSE COM-
              PANION OF 17.5M.
V466   CYG    MIN II 11.4.
V469   CYG    MIN II 12.9; MIN II - MIN I =0.57P.
V470   CYG    MIN II 8.545.
V471   CYG    S 5.5/5.5.
V473   CYG    P VAR. MAX=2430615+218.5D*E (J.D.2418000-31000)
               0346!; OCE/SINCE J.D.2442300-CM. TA./SEE TABLE.
V474   CYG    D=0.014P.
V477   CYG    MIN II 8.69; D II =0.09P; D=0.003P. P VAR. MIN I =
              =2429194.309+2.3470011D*E (J.D.2410000-29200)
               0001!; MIN I =2437317.2695+2.3469943D*E (J.D.
              2429200-39700)  8919!; OCE/SINCE J.D.2439700-CM.
              TA./SEE TABLE.
              BPAEHE H AC C =349 ET;/APSIDAL MOTION
              WITH =349 YEARS; E=0.302  6175!. 0.331P (1965-1970)<=
              <=MIN II - MIN I <=0.460P (1904).
V478   CYG    VB A (B 12.8M, 4", 259G). MIN II 9.02; MIN II - MIN I =
              =0.5072P.
V482   CYG    VB A (B 14.4M V, M4 III, 8", 225G).
V483   CYG    MIN II 11.9.
V484   CYG    MIN II 13.6.
V486   CYG    MIN II 14.3.
V488   CYG    MIN II 13.0.
V490   CYG    MIN II 13.5; MIN II - MIN I =0.47P.
V491   CYG    MIN II 14.7.
V493   CYG    MIN II 12.9.
V494   CYG    MIN II 13.6.
V496   CYG    MIN II 12.5.
V498   CYG    MIN II 10.27.
V500   CYG    VB B (A 11.5M; 18", 45G). MIN II 12.0.
V501   CYG    MIN II 13.1; D=0.02P.
V502   CYG    MIN II 14.2.
V505   CYG    MIN II 12.0.
V509   CYG    D=0.05P.
V512   CYG    MIN II 11.5. EMEHT COEPAT CHCOAH
              EH:/THERE IS A PERIODIC TERM IN THE ELEMENTS:+0.065D*
              *SIN 0.2105263G (E+538).
V513   CYG    MIN II 12.6.
V519   CYG    MIN II 13.4.
V520   CYG    VB A (B 15", 135G).
V525   CYG    D=0.03P:.
V526   CYG    MIN II 13.1. B PAOHE PACCEHHOO CKOEH/IN THE
              REGION OF THE OPEN CLUSTER TGC 7039.
V532   CYG    P VAR. MAX=2434618.158+3.283651D*E (J.D.2427900-
              35000); MIX=2436817.694+3.282792D*E (J.D.2435000-
              38700); OCE/SINCE J.D.2438700-CM. TA./SEE
              TABLE.
V536   CYG    D=0.010P.
V538   CYG    B-V:+1.17, +1.50.
V539   CYG    P2=1500D.
V541   CYG    MIN II 10.9; D II =0.012P; MIN II - MIN I =0.453P.
V544   CYG    P VAR?
V546   CYG    MIN II 15.2:; MIN II - MIN I =0.48P; D=0.077P. B TEMHO
              TMAHHOCT/IN THE DARK NEBULA BARNARD 144.
V547   CYG    B-V: +1.27, +1.73. B TEMHO TMAHHOCT/IN THE DARK
              NEBULA BARNARD 144.
V548   CYG    MIN II 8.62. P VAR. MIN I =2442279.3838+1.80524695D*E
              (J.D.2430800-42300)  8930!; OCE/SINCE J.D.2442300-
              CM. TA./SEE TABLE.
V563   CYG    P VAR. MAX=2427590+295.4D*E (J.D.2426000-30250);
              OCE/SINCE J.D.2430250-CM. TA./SEE TABLE.
V567   CYG    D=0.036P.
V581   CYG    KPACHA/RED.
V586   CYG    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF THE
              OPEN CLUSTER NGC 7039.
V588   CYG    VB A (B 18M, 15", 0G). OEH KPACHA/VERY RED.
V589   CYG    VB.
V606   CYG    P VAR. MAX=2428376.7+50.245D*E (J.D.2427950-
              31330)  1262!; OCE/SINCE J.D.2437100-CM. TA./
              SEE TABLE.
V612   CYG    K/CYCLES OF 50-100D (J.D.2427950-31330)  1262!;
              OCE/SINCE J.D.2437100-CM. TA./SEE TABLE.
V614   CYG    MIN II 14.5.
V618   CYG    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF THE
              OPEN CLUSTER TGC 7092.
V622   CYG    CM./SEE V618 CYG.
V628   CYG    MIN II 12.5.
V635   CYG    MIN II 13.5.
V643   CYG    P VAR. EMEHT, AHHE B TAE, CPABEB B
              HTEPBAE J.D.2427950-31330./ELEMENTS GIVEN IN THE
              TABLE ARE VALID IN THE INTERVAL J.D.2427950-31330.
V644   CYG    VB A (B 15.6M, 6", 141G; C 16.3M, 6", 141G).
V645   CYG    HAAETC KAK PK CCTOK TMAHHOCT AMET-
              POM-2", PACCEBAE EHE CBAHHO C HE,
              HO HEBMO -A OOEH BE KACCA O8.
              COCTABHA ACT CHO OPOBAHHO OPHO
              TMAHHOCT PAMEPOM OKOO 10". B CEKTPE - C-
              HE MCC H, FE II,  O I!,  S II!  P.  8942, 9129!.
              CTOHK MAEPHOO EH H2O. CTOHK H-
              PAKPACHOO EH CRL 2789./OBSERVED AS THE
              BRIGHT NEBULAR CONDENSATION WITH-2" DIAMETER SCAT-
              TERING LIGHT OF AN O8 STAR ASSOCIATED WITH IT BUT INVI-
              SIBLE BECAUSE OF ABSORPTION. A PART OF STRONGLY POLARI-
              ZED BIPOLAR NEBULA WITH DIAMETER ABOUT 10". THERE ARE
              STRONG EMISSION LINES OF H, FE II,  O I!,  S II!, ETC. IN
              THE SPECTRUM  8942, 9129!. H2O MASER SOURCE. INFRA-
              RED SOURCE CRL 2789.
V651   CYG    MIN II 14.7.
V652   CYG    MIN II 12.1.
V664   CYG    D=0.05P.
V666   CYG    P VAR. MAX=2427965+236D*E (J.D.2427950-31350)
               1262!; OCE/SINCE J.D.2433400-CM. TA./SEE
              TABLE.
V670   CYG    SP EH TECHO AP./SP COMPONENT OF A CLOSE BINARY.
V680   CYG    MIN II 10.3.
V685   CYG    VB.
V687   CYG    MIN II 10.4. P VAR?
V688   CYG    D=0.029P.
V690   CYG    D=0.021P.
V691   CYG    D<=0.034P.
V692   CYG    MIN II 14.9?
V693   CYG    MIN II 14.4?
V694   CYG    D=0.017P.
V695   CYG    31 CYG. O-BMOM, OPAET EH CCTEM C
              V1488 CYG (32 CYG)./PROBABLY ENTERS A COMMON SYSTEM
              WITH V1488 CYG (32 CYG).
              VB A (B 13.0M, 36.8", 332G; C 6.99M, 107.0", 174G; D 5.0M,
              338", 323G). D=0.0151P.
              HTEPEPOMETPECKA BOHA ATMEHHA CCTEMA
              (A=0.08", E=0.15  1582!; 0.035", 141.8G, 1980.4). B
              TAE PBEEHA OXA ATMEH KOMOHEHTA CEKT-
              PAHOO KACCA B4 KOMOHEHTOM KACCA K4. AM-
              TA CHO MEHETC B ABCMOCT OT H BO-
              H: A (LAMBDA 6560 A)=0.03M, A (LAMBDA 3530 A)=1.80M      ./IN-
 9131!
              TERFEROMETRIC BINARY ECLIPSING SYSTEM (A=0.08", E=0.15
               1582!; 0.035", 141.8G, 1980.4). THE EPOCH OF ECLIPSE OF
              THE COMPONENT OF THE SPECTRAL TYPE B4 BY THE COMPO-
              NENT OF THE TYPE K4 IS GIVEN IN THE TABLE. THE AMPLI-
              TUDE STRONGLY VARIES DEPENDING UPON THE WAVELENGTH:
              A(LAMBDA 6560 A)=0.03M, A(LAMBDA 3530 A)=1.80M  9131!.
V696   CYG    CPEH BEHA MEHETC C P=1600D./MEAN MAGNI-
              TUDE VARIES WITH P=1600D.
V700   CYG    MIN II 12.3. P VAR. MIN I =2432028.863+0.340047D*E
              (J.D.2431700-37500)  5352!; OCE/SINCE J.D.
              2437500-CM. TA./SEE TABLE.
V704   CYG    MIN II 14.2.
V706   CYG    MIN II 13.9.
V713   CYG    MIN II 15.1.
V720   CYG    P VAR. MIN I =2427611+332D*E (J.D.2429450-32000)
               0798!; OCE/SINCE J.D.2432500-CM. TA./SEE
              TABLE.
V726   CYG    MIN II 12.8; D=0.018P.
V728   CYG    P VAR. MIN=2425760.475+2.0601256D*E (J.D.2425500-
              35000)  0164!; OCE/SINCE J.D.2439700-CM. TA./
              SEE TABLE.
V729   CYG    VB A (B 13.5M, 1.5", 65G). MIN II 9.29. P VAR. MIN I =
              =2434264.638+6.597700D*E (J.D.2428700-37900)
               0001!; OCE/SINCE J.D.2439750-CM. TA./SEE
              TABLE.
V731   CYG    VB.
V735   CYG    HA MIN II/DEPTH OF MIN II 0.04M.
V736   CYG    MIN II 16.5. HEAEKO OT NQ CYG./CLOSE TO NQ CYG.
V737   CYG    BEA/STAR 23-50  1321!.
V739   CYG    BEA/STAR 36-81  1321!.
V741   CYG    D=0.03P.
V742   CYG    P VAR. MAX=2429409.448+0.93979D*E (J.D.2428420-
              30700)  8977!; MAX=2431489.580+0.94010D*E (J.D.
              2430250-32350); MAX=2433282.014+0.93979D*E (J.D.
              2432350-33650); OCE/SINCE J.D.2433650-CM. TA./
              SEE TABLE.
              COACHO  8977! OCE J.D.2430700 HAEH -
              E PECTABTC EMEHTAM:/ACCORDING TO  8977!
              SINCE J.D.2430700 THE OBSERVATIONS ARE BETTER REPRE-
              SENTED BY THE ELEMENTS: MAX=2432943.701+0.93977897D*E-
              -1.067D*10**-7*E**2.
V747   CYG    HTEPBA ME MAKCMMAM ECKA - 2000-4000D.
              HE KPACHA./THE INTERVALS BETWEEN MAXIMA OF BRIGHTNESS
              ARE 2000-4000D. NOT RED.
V751   CYG    B PAOHE TMAHHOCT/IN THE REGION OF THE NEBULA
              IC 5070. SB (P=0.25D  9132!).
              HA CTPE HEOE KOEAH B PAOHE MAKCM-
              MA ECKA (<B-V>=+0.25) HOA HAKABATC
              OKE MHMM, EC HECKOKO COTEH HE
               2699!. CTOHK MKOO PEHTEHOBCKOO EH
               9133!. OCAHE CEKTPA  2698, 9132!./RAPID SMALL
              VARIATIONS NEAR MAXIMUM OF BRIGHTNESS (<B-V>=+0.25)
              ARE SUPERIMPOSED SOMETIMES BY DEEP MINIMA LASTING
              FOR SOME HUNDREDS DAYS  2699!. SOFT X-RAY SOURCE
               9133!. SPECTRUM DESCRIPTION  2698, 9132!.
V752   CYG    <B-V>=+0.77, <U-B>=-0.47.
V753   CYG    D=0.12P. P=0.952374D?
V757   CYG    KPACHA/RED.
V758   CYG    P=400D?
V759   CYG    P VAR. MAX=2434513.427+0.36001476D*E (J.D.
              2414430-34570)  3506!; OCE/SINCE J.D.2434500-
              CM. TA./SEE TABLE.
              EKT AKO./BLAZHKO EFFECT.
V779   CYG    T/TYPE RR?
V781   CYG    P VAR?
V783   CYG    P VAR. MAX=2433261.029+0.62069487D*E (J.D.2424690-
              34000); OCE/SINCE J.D.2438970-CM. TA./SEE
              TABLE.
V786   CYG    OHO B MHMME ECKA C CTPM OPAH-
              M HA 0.5M-1.0M. B HTEPBAE J.D.2427692-697 A
              13.5M./USUALLY IN MINIMUM BRIGHTNESS, WITH RAPID
              BRIGHTENINGS BY 0.5M-1.0M. IN THE INTERVAL J.D.2427692-
              697 THE BRIGHTNESS WAS 13.5M.
V789   CYG    P VAR?  FE/H!=-0.91.
V795   CYG    SF KOMOHEHT TECHO AP./SF COMPONENT OF A CLOSE
              PAIR.
V796   CYG    MIN II 11.4.
V797   CYG    MIN 15.4.
V799   CYG    P VAR.
V801   CYG    EMEHT COEPAT KBAPATH EH:/THERE IS A
              SQUARE TERM IN THE ELEMENTS:+1.93D*10**-10*E**2.
V802   CYG    P VAR. MAX=2432779.9342+0.59560377D*E (J.D.
              2425480-35170)  2775!; MAX=2439415.263+
              +0.5955638D*E (J.D.2435950-40000)  9266!. MAX=
              =2440036.409+0.595447D*E (J.D.2440000-41000); MAX=
              =2441517.498+0.595635D*E (J.D.2441000-42500); O-
              CE/SINCE J.D.2442500-CM. TA./SEE TABLE.
              OPMA KPBO ECKA MEHETC (0.13P<=M-M<=0.50P);
              MEHEH EPOA HOA COPOBOATC CH-
              M MEHEHM AMT (B HTEPBAE J.D.
              2440000-41000 0.3M<=A<=1.7M)./SHAPE OF THE LIGHT CURVE
              VARIES (0.13P<=M-M<=0.50P); PERIOD VARIATIONS ARE ACCOM-
              PANIED SOMETIMES BY STRONG VARIATIONS OF AMPLITUDE (IN
              THE INTERVAL J.D.2440000-41000; 0.3M<=A<=1.7M).
V803   CYG    MIN II 14.5.
V806   CYG    MIN II 15.0; D II =0.061P.
V807   CYG    MIN II 14.9.
V808   CYG    ECK B MAKCMME MEHETC./BRIGHTNESS IN MAXIMUM
              VARIES.
V809   CYG    MIN II 13.6; D II =0.069P.
V810   CYG    D=0.050P. HA MIN II/DEPTH OF MIN II 0.05M. P VAR?
V817   CYG    SP KOMOHEHT AP./SP COMPONENT OF THE PAIR.
V818   CYG    OPMA KPBO ECKA  EPO MEHTC./THAPE OF
              THE LIGHT CURVE AND PERIOD VARY.
V821   CYG    MIN II 15.6.
V822   CYG    MIN II 13.0.
V824   CYG    MIN II 14.3.
V825   CYG    MIN II 16.9. MIN II =2433871.915+7.709015D*E.
V826   CYG    MIN II 14.7.
V828   CYG    MIN II 10.12.
V832   CYG    VB A (B 9.43M, 20", 352G; C 11.62M, 27", 141G; D 12.72M,
              38", 220G). OCAHE MEHEH B CEKTPE/DESCRIP-
              TION OF SPECTRAL VARIATIONS  9135!.
V836   CYG    MIN II 8.77. P VAR. MIN I =2426547.5224+0.65341090D*E
              (J.D.2425500-42000)  3869!; OCE/SINCE J.D.
              2441200-CM. TA./SEE TABLE.
              OPMA KPBO ECKA MEHETC./THAPE OF THE LIGHT
              CURVE VARIES.
V840   CYG    LS II 28.3G  8090!. K/CYCLES 250-300D.
V841   CYG    MIN II 11.2.
V842   CYG    MIN II 14.1.
V844   CYG    VB A (B 17.8M, 2.9", 50G).
V850   CYG    MIN II 11.8. P VAR. MIN I =2430587.263+4.5578D*E (J.D.
              2428750-30590)  4253!; OCE/SINCE J.D.2434330-
              CM. TA./SEE TABLE.
V851   CYG    D=0.017P?
V852   CYG    MIN II 14.9.
V853   CYG    MIN II 14.2.
V856   CYG    HA MIN II/DEPTH OF MIN II 0.05M.
V857   CYG    HA MIN II/DEPTH OF MIN II 0.03M.
V859   CYG    MIN II 12.1.
V865   CYG    MIN II 14.6.
V866   CYG    MIN II 13.9.
V869   CYG    MIN II 14.8. OPMA KPBO ECKA MEHETC./THAPE
              OF THE LIGHT CURVE VARIES.
V870   CYG    MIN II 15.8.
V871   CYG    MIN II 14.9.
V873   CYG    MIN II 14.7. MIN II - MIN I =0.48P.
V874   CYG    MIN II 13.8.
V877   CYG    MIN II 12.9.
V880   CYG    MIN II 14.1; MIN II - MIN I =0.506P; D=0.02P.
V881   CYG    DS HEOOE/DS IS SMALL  9037!.
V882   CYG     FE/H!=-1.42.
V884   CYG    NP KOMOHEHT AP/NP COMPONENT OF A PAIR. MIN II
              14.2.
V885   CYG    MIN II 10.2.
V886   CYG    MIN II 14.1; MIN II - MIN I =0.515P.
V887   CYG    HA MIN II/DEPTH OF MIN II 0.03M.
V888   CYG    MIN II 15.9.
V889   CYG    MIN II 10.4.
V891   CYG    MIN II 9.4.
V892   CYG    MIN II 15.5. NF KOMOHEHT TECHO BOHO./NF COMPO-
              NENT OF A CLOSE PAIR.
V900   CYG    MIN II 15.2.
V902   CYG    D=0.02P. HA MIN II/DEPTH OF MIN II 0.05M.
V906   CYG    MIN II 15.7.
V907   CYG    MIN II 14.9. COACHO/ACCORDING TO  4427! MIN I =
              =2435066.257+0.54138554D*E.
V908   CYG    NF KOMOHEHT TECHO AP. HA MIN II 0.04M./
              NF COMPONENT OF A CLOSE PAIR. DEPTH OF MIN II 0.04M.
V909   CYG    MIN II 9.66.
V910   CYG    MIN II 14.2; D=0.02P.
V911   CYG    MIN II 14.6. P VAR? MIN I =2432120.251+3.42262215D*E
              (J.D.2415500-37900)  4761!; OCE/SINCE J.D.
              2437100-CM. TA./SEE TABLE.
V912   CYG    HA MIN II/DEPTH OF MIN II 0.05M.
V913   CYG    VB A (B 17M, 0G).
V920   CYG    A VAR. EKT AKO?/BLAZHKO EFFECT?
V922   CYG    D=0.02P:.
V924   CYG    P VAR. MAX=2435706.776+5.5709816D*E (J.D.2432760-
              38000)  8053!; OCE/SINCE J.D.2438000-CM. TA./
              SEE TABLE.
V925   CYG    MIN II 16.0.
V927   CYG    AHA OXA MIN ECKA./EPOCH OF MIN BRIGHTNESS IS
              GIVEN.
V928   CYG    MIN II 15.4.
V931   CYG    MIN II 14.5.
V932   CYG    HA MIN II/DEPTH OF MIN II 0.04M.
V934   CYG    MIN II 13.7.
V936   CYG    HA MIN II/DEPTH OF MIN II 0.05M.
V939   CYG    MIN II 12.5.
V940   CYG    MIN II 15.1.
V941   CYG    MIN II 13.2.
V942   CYG    VB A (B-10G, C-110G).
V944   CYG    NP KOMOHEHT AP./NP COMPONENT OF PAIR.
V947   CYG    MIN II 15.0.
V948   CYG    MIN II 15.2.
V949   CYG    KPACHA./RED.
V955   CYG    MIN II 15.3. SP KOMOHEHT TECHO AP./SP COMPO-
              NENT OF A CLOSE PAIR.
V956   CYG    MIN II 15.1. SP KOMOHEHT TECHO AP./SP COMPO-
              NENT OF A CLOSE PAIR.
V957   CYG    MIN II 12.6.
V958   CYG    P=199D?
V959   CYG    MIN II 11.4; MIN II - MIN I =0.52P; D II =0.16P:.
              SP KOMOHEHT TECHO AP./SP COMPONENT OF A CLOSE
              PAIR.
V961   CYG    MIN II 12.4; MIN II - MIN I =0.505P.
V962   CYG    D=0.02P:.
V964   CYG    MIN II 14.4.
V965   CYG    MIN II 14.9. T/TYPE RRC? P=0.32028628D?
V970   CYG    MIN II 14.8.
V974   CYG    MIN II 12.5; MIN II - MIN I =0.462P. MIN II =2435373.398+
              +3.204418D*E.
V979   CYG    MIN II 14.7.
V981   CYG    MIN II 15.0.
V997   CYG     FE/H!=-0.77.
V997   CYG     FE/H!=-0.77.
V1004  CYG    MIN II 13.0.
V1007  CYG    CM./SEE V932 CYG.
V1008  CYG    MIN II 16.0.
V1010  CYG    HA MIN II/DEPTH OF MIN II 0.03M.
V1011  CYG    CM./SEE V932 CYG.
V1012  CYG    MIN II 15.4.
V1016  CYG    O BCK 1964. ECK MEHC B PEEAX 15.0-
              17.5PG  5701!, CEKTPAH KACC - OH ME ALFA
               1222!. B 1964-67 . POOO BEEHE EC-
              KA OT 16.0M O 11.2M B. B 1967-79 . ECK OCTE-
              EHHO BOPOC OT 11.2M O 10.05M B, B CCTEME V OC-
              TABAC OCTOHHM (10.5M). B HPAKPACHO O-
              ACT MEHETC B PEEAX 6.9-8.4 J, 4.7-5.8 K C
              EPOOM 470D  7174, 9141!. MCCOHH CEKTP
              BCOKOO BOEH C MOHM HPAKPACHM
              TKOM OOEH CEKTP CMOTECKX EPE-
              MEHHX  9142!. CTOHK PEHTEHOBCKOO  PAO-
              EH./BEFORE THE OUTBURST IN 1964 THE BRIGHTNESS
              CHANGED BETWEEN 15.0M AND 17.5M PG  5701!, THE SPECT-
              RAL TYPE WAS LATE ME ALFA  1222!. IN THE 1964-67 THE
              BRIGHTNESS INCREASED FROM 16.0M TO 11.2M B. IN 1967-
              69 THE BRIGHTNESS STEADILY INCREASED TO 10.05M B,
              BEING CONSTANT IN V SYSTEM (10.5M). IN THE INFRARED IT
              CHANGES IN THE LIMITS 6.9-8.4 J, 4.7-5.8 K WITH THE
              PERIOD 470D  7174, 9141!. HIGH EXCITATION EMISSION
              SPECTRUM WITH STRONG IR EXCESS RESEMBLES THAT OF
              SYMBIOTIC VARIABLES  9142!. X-RAY AND RADIO SOURCE.
V1018  CYG    MIN II 11.6.
V1021  CYG    MIN II 14.3.
V1023  CYG    MIN II 12.9; D=0.03P:. D II =0.14P. MIN II - MIN I =0.495P.
V1024  CYG    CM./SEE V932 CYG.
V1030  CYG    PBEEHHE B TAE EMEHT ECTBT B H-
              TEPBAE J.D.2426600-32300./ELEMENTS GIVEN IN THE
              TABLE ARE VALID IN THE INTERVAL J.D.2426600-32300.
V1033  CYG    P VAR.
V1034  CYG    MIN II 9.9.
V1035  CYG    P VAR?
V1037  CYG    MIN II 14.8.
V1038  CYG    VB B (9.4", 215G, 1963). MIN II 15.5.
V1039  CYG    MIN II 15.6.
V1042  CYG    VB A (B 10M, 53", 110G). B OACT H II/IN H II RE-
              GION S 109.
V1044  CYG    MIN II 16.5.
V1045  CYG    MIN II 16.0.
V1047  CYG    D=0.02P.
V1053  CYG    D=0.05P.
V1057  CYG    B TEMHO TMAHHOCT, B PAOHE TMAHHOCT CEBEP-
              HA AMEPKA (NGC 7000). B 1969-70 . (J.D.
              2440400-830) POOA BCKA OT 16.5M O 10.3M.
              MAX ECKA OCTHT B J.D.2440830 (CEKTP B3).
              O BCK ECK MEHC B PEEAX 15.5M-16.5M,
              CEKTP-KE C XAPAKTEPHM PHAKAM BE TA
              T TAU  2698, 6415!. OCE BCK ECK HAA MO-
              HOTOHHO OCAEBAT, OCTHB B 1982. BEH
              13.1M B (CEKTP - G2-G5IB). C 1971.-CHA MC-
              C B H ALFA. HAATC TAKE HEOE CTPE
              KTA ECKA. OCAHE MEHEH ECKA
               6504, 7115, 7754, 8996!. BEA CBAHA C OO-
              PAHO CBETO OTPAAE TMAHHOCT HO
              -3', OBBEC B 1971., PKOCT KOTOPO
              MEHAETC O MEPE OCAEH ECKA BE.
              HAATC BCK MAEPHO MCC OH./IN
              THE DARK NEBULA, IN THE REGION OF THE NORTH AMERICA
              NEBULA (NGC 7000). IN 1969-70 (J.D.2440400-830)
              THE OUTBURST FROM 16.5M TO 10.3M OCCURED. BRIGHTNESS
              MAXIMUM WAS OBSERVED AT J.D.2440830 (SPECTRUM-
              B3). BEFORE THE OUTBURST THE LIGHT CHANGED IN THE RANGE
              15.5M-16.5M, THE SPECTRAL TYPE WAS KE WITH CHARACTE-
              RISTIC FEATURES OF T TAU TYPE STARS  2698, 6415!. AF-
              TER THE OUTBURST THE BRIGHTNESS BEGAN TO WEAKEN MO-
              NOTONOUOSLY AND IN 1982 REACHED 13.1M B (THE SPECT-
              RAL TYPE ABOUT G2-G5 IB). STRONG H ALFA EMISSION APPEA-
              RED IN 1971. THERE ARE ALSO SMALL RAPID LIGHT FLUCTUA-
              TIONS. DESCRIPTION OF LIGHT VARIATIONS  6504, 7115,
              7754, 8996!. THE STAR IS ASSOCIATED WITH A LUMINOUS
              ARC-SHAPED REFLECTION NEBULA. THIS NEBULA WITH LENGTH
              OF ABOUT 3' APPEARED IN 1971 AND ITS BRIGHTNESS IS
              GRADUALLY DECREASING SIMULTANEOUSLY WITH THE FADING
              OF THE STAR.
V1061  CYG    MIN II 9.5.
V1063  CYG    P VAR. MAX=2428260+339D*E (J.D.2428260-30700);
              OCE/SINCE J.D.2433500-CM. TA./SEE TABLE.
V1064  CYG    MIN II 15.3.
V1068  CYG    MIN II 11.2; D=0.070P. BHE ATMEH HAAETC
              MPPA CTOPCOHHA BOHA C AMHO
              -0.1M V  8999!./A MIGRATING WAVELIKE DISTORSION WITH
              AN AMPLITUDE-0.1M V IS BEING OBSERVED OUTSIDE EC-
              LIPSES  8999!.
V1073  CYG    MIN II 8.57.
V1074  CYG    MIN II 14.8.
V1083  CYG    MIN II 11.2.
V1085  CYG    HAEH, PBEEHHE B  7010!, POTBOPEAT
              EMEHTAM, AHHM B  7193!:/OBSERVATIONS GIVEN IN
               7010! CONTRADICT THE ELEMENTS GIVEN IN  7193!: MIN=
              =2437856.592+2.8089D*E.
V1096  CYG    D=0.03P.
V1102  CYG    N-AAKTKA E PAOEH. CEKTP ACOP-
              OHH, MCCOHHX H HET./RADIO-QUIET N GA-
              LAXY. ABSORPTION SPECTRUM WITHOUT EMISSION LINES;
              Z=0.0272.
V1111  CYG    BOMOEH EKT AKO./BLAZHKO EFFECT IS POS-
              SIBLE.
V1122  CYG    CM./SEE V1111 CYG.
V1130  CYG    MIN II 12.9.
V1136  CYG    MIN II 13.2. OPTA KCEHTPHA (E=0.3). BOMO-
              HO BPAEHE H AC  8051!./ECCENTRIC ORBIT (E=
              =0.3). APSIDAL MOTION IS POSSIBLE  8051!.
V1141  CYG    MIN II 11.8.
V1142  CYG    MIN II 13.4.
V1143  CYG    MIN II 6.06; MIN II - MIN I =0.743P; D=0.002P.
V1157  CYG    MIN II 13.6.
V1158  CYG    D=0.02P; CM./SEE V932 CYG.
V1161  CYG    D=0.01P.
V1162  CYG    HAAC TOKO OH MAX (CM. TA.). OCE
              TOO  HE BHA,  OT OCTOHHA (17.6M-
              17.8M). OOBATA./ONLY ONE MAX WAS OBSERVED
              (SEE TABLE). THERE AFTER - EITHER INVISIBLE, OR FAIRLY
              CONSTANT (17.6M-17.8M). BLUISH.
V1171  CYG    VB A (B 11.0M, 0.34", 71.2G; 1979.5). MIN II 10.3.
V1175  CYG    MIN II 16.5. P VAR. MIN I =2434629.545+1.3330D*E
              (J.D.2426620-34630); OCE/SINCE J.D.2434635-
              CM. TA./SEE TABLE.
V1176  CYG    VB. EPEMEHHM, BEPOTHO, BETC CEBEPH
              KPACH KOMOHEHT./VARIABLE IS PROBABLY THE
              NORTHERN RED COMPONENT.
V1187  CYG    B TMAHHOCT/IN THE NEBULA IC 1318B. MIN II 11.19.
              P=3.7675D?
V1188  CYG    MIN II 14.3.
V1189  CYG    MIN II 13.7. P VAR. MIN I =2437906.516+1.041908D*E
              (J.D.2426620-31240); OCE/SINCE J.D.2437906-
              CM. TA./SEE TABLE.
V1191  CYG    B TMAHHOCT/IN THE NEBULA IC 1318B. VB A (B 13M,
              11", 299G; C 13M, 11", 284G). MIN II 11.11.
              OPMA KPBO ECKA MEHETC./SHAPE OF THE LIGHT
              CURVE VARIES.
V1193  CYG    MIN II 14.3.
V1196  CYG    CM./SEE V936 CYG.
V1200  CYG    MIN II 16.1:.
V1210  CYG    KPACHA./RED.
V1212  CYG    CM./SEE V1210 CYG.
V1218  CYG    VB A (B 17M, SF).
V1225  CYG    VB A (B 16M V, B-V=+1.3M, 1.2", 270G; C 15.0M V,
              B-V=+0.5M, 2.4", 270G); P VAR? MAX=2428250+
              +384.2D*E (J.D.2428200-38250)  3160!; OCE/SINCE
              J.D.2438500-CM. TA./SEE TABLE.
V1236  CYG    KPACHA./RED.
V1255  CYG    ECK B MAX MEHETC B PEEAX 15.2M-16.0M C BO-
              MOHM EMEHTAM:/BRIGHTNESS IN MAX VARIES IN
              THE RANGE 15.2M-16.0M WITH POSSIBLE ELEMENTS: MAX=
              =2439382.281+0.28619537D*E.
V1256  CYG    MIN II 14.1.
V1273  CYG    MIN II 16.5.
V1275  CYG    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF THE
              OPEN CLUSTER NGC 6819.
V1281  CYG    MIN II 15.4.
V1285  CYG    KPACHA./RED.
V1302  CYG    CM./SEE V936 CYG.
V1305  CYG    MIN II 11.5M-11.7M (VAR).
V1307  CYG    CEPC TOEK CPEHE KPBO ECKA HATE-
              HA./CONSIDERABLE DISPERSION OF MEAN LIGHT CURVE
              POINTS.
V1315  CYG    MIN II 15.3.
V1316  CYG    (P)>100D.
V1318  CYG    LKH ALFA 225. CM./SEE V1331 CYG.
V1321  CYG    P=0.7281802D?
V1322  CYG    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6913.
V1326  CYG    MIN II 11.8; MIN II - MIN I =0.53P.
V1327  CYG    OEH KPACHA/VERY RED.
V1329  CYG    B 1891-1964 . MEHEH ECKA B PEEAX 14.2M-
              15.5M C OKM MHMMAM O 18M, OBETBO-
              PM EMEHTAM, PBEEHHM B TAE; D=0.1P;
              CEKTPAH KACC-M  7235!. B 1964.-BC-
              KA O 12.1M. ATEM - OCTEEHHOE AEHE ECKA,
              HA KOTOPOE HAKABATC EPOECKE KOEA-
              H C AMTO OKOO 1M. MHMM ECKA O-
              PEHEM OBETBOPT PBEEHHM B TAE
              EMEHTAM, HO XAPAKTEP ATMEH MEHC, BO-
              MOHO, BCECTBE OBEH OTHO OOOK,
              BPOEHHO OHM  KOMOHEHTOB. OCE BC-
              K HAAETC MCCOHH CEKTP BCOKOO BO-
              EH C HPAKPACHM TKOM, OOH
              CEKTP CMOTECKX EPEMEHHX./IN 1891-1964
              LIGHT VARIATIONS IN THE RANGE 14.2M-15.5M WITH DEEP
              MINIMA TO 18M; THE MINIMA ARE SATISFIED BY THE ELE-
              MENTS GIVEN IN THE TABLE; D=0.1P; SPECTRAL TYPE M
               7235!. IN 1964-THE OUTBURST UP TO 12.1M. THEN GRA-
              DUAL BRIGHTNESS DECREASE SUPERIMPOSED BY PERIODICAL
              VARIATIONS WITH AN AMPLITUDE NEAR 1M. LIGHT MINIMA
              AS BEFORE ARE SATISFIED BY THE ELEMENTS GIVEN IN THE
              TABLE BUT THE CHARACTER OF ECLIPSES CHANGED (PROBABLY
              BECAUSE OF APPEARANCE OF A DENSE ENVELOPE EJECTED
              BY ONE OF THE COMPONENTS OF THE SYSTEM). AFTER THE
              OUTBURST HIGH EXCITATION EMISSION SPECTRUM WITH IR
              EXCESS IS OBSERVED SIMILAR TO THE SPECTRUM OF SYM-
              BIOTIC VARIABLES.
V1331  CYG    CBAHA C KOMETOOPAHO TMAHHOCT./ASSOCIA-
              TED WITH A COMETARY NEBULA.
V1334  CYG    VB A (B 7.9M, B5-B8, 0.13", 26.1G, 1975).
V1336  CYG    COACHO/ACCORDING TO  7010!, RR? P=0.5D?
V1341  CYG    CYG X-2. SB 1. O'EKT CEPECKO COCTABE
              (NU=-220 KM/C). CH EKT OTPAEH PBO-
              T K MEHEH CEKTPAHOO KACCA F-KOMO-
              HEHTA. PO CEKTPAHX H MEHTC. -
              H HE II, KCA II, C III, N III - B MCC. HAAT-
              C COKOHOE  AKTBHOE COCTOH CCTEM. B CO-
              KOHOM COCTOH CPEH KPBA ECKA - BOHA
              BOHA CO CPEHM PEEAM MEHEH ECKA
              15.1M-15.4M B. B MIN I, PBEEHHOM B TAE, F-
              KOMOHEHT HAXOTC B BEPXHEM COEHEH; MIN II
              15.4. ATMEHE AKKPEOHHOO CKA P AE 0.5P-
              ACTHOE. HAKABAETC CTPA EPEMEHHOCT
              ECKA HA 0.1M A 10 MHT  O 0.5M A HECKOKO
              ACOB. B AKTBHX COCTOHX, XC-10D,
              CPEH ECK BOPACTAET HA 0.5M. PAOCTOHK
              HA ACTOHE 8085 M, CTOHK MKOO  ECTKOO
              PEHTEHOBCKOO EH OT 0.1 O 60 KB./HALO
              OBJECT (NU=-220 KM/S). STRONG REFLECTION EFFECT CHANGES
              THE SPECTRAL TYPE OF THE F COMPONENT. SPECTRAL LINE PRO-
              FILES VARY. THE LINES OF HE II, KCA II, C III,AND N III
ARE
              IN EMISSION. THE SYSTEM HAS LOW AND HIGH STATES. DU-
              RING THE LOW STATE THE MEAN LIGHT CURVE IS A DOUBLE
              WAVE WITH THE RANGE 15.1M-15.4M B. EPOCH OF MIN I GI-
              VEN IN THE TABLE CORRESPONDS TO THE F STAR IN SUPE-
              RIOR CONJUNCTION; MIN II 15.4. THE ECLIPSE OF THE AC-
              CRETION DISK AT THE PHASE 0.5P IN PARTIAL. RAPID LIGHT
              VARIABILITY BY 0.1M IN 10 MINUTES AND BY 0.5M IN SEVE-
              RAL HOURS IS SUPERIMPOSED. IN THE HIGH STATES LASTING
              FOR-10D THE MEAN LIGHT INCREASES BY 0.5M. RADIO
              SOURCE AT 8085 MHZ, SOURCE OF SOFT AND HARD X-RAY
              EMISSION FROM 0.1 TO 60 KEV.
V1345  CYG    MIN II 15.0:.
V1354  CYG    CM./SEE V932 CYG.
V1356  CYG    MIN II 10.4.
V1357  CYG    CYG X-1. SB1. B TAE - OXA HHEO COE-
              HEH OTECKOO KOMOHEHTA. MIN II 8.88. OPMA
              KPBO ECKA MEHETC; MIN II HOA HE HACTA-
              T. BOMOHA EPOECKA COCTABA B -
              MEHEH OPM KPBO ECKA  OPA C P=
              =78.4D  9021, 9022!. CTPO EPEMEHH PEHTEHOB-
              CK CTOHK B POKOM AAOHE O 3MB, XAPAK-
              TEPC CMEHO COKOHX  AKTBHX CO-
              CTOH. OHAPEHO TAKE MEHEHE ECKA 
              PEHTEHOBCKOO EH C P=294D  9154, 9156!.
              EPEMEHH  BCXBA PAOCTOHK HA A-
              CTOTAX 2695  8085 M./THE EPOCH OF THE INFERIOR
              CONJUNCTION OF THE OPTICAL COMPONENT IS GIVEN IN THE
              TABLE. MIN II 8.88. THE SHAPE OF THE LIGHT CURVE VA-
              RIES; MIN II SOMETIMES ARE NOT OBSERVED. THE PERIO-
              DICITY IN THE LIGHT CURVE VARIATIONS AS WELL AS IN PO-
              LARIZATION CHANGES IS POSSIBLE WITH P=78.4D  9021,
              9022!. RAPIDLY VARIABLE X-RAY SOURCE IN WIDE RANGE
              UP TO 3 MEV CHARACTERIZED BY THE CHANGE OF HIGH AND
              LOW STATES. LIGHT AND X-RAY VARIATION WITH P=294D
              IS ALSO DETECTED  9154, 9156!. VARIABLE AND FLARE RA-
              DIO SOURCE AT 2695 AND 8085 MHZ.
V1372  CYG    P2=360D?.
V1374  CYG    MIN II 17.7.
V1384  CYG    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6913.
V1396  CYG    VB AB (10.26M V, 12.3M V; A=0.1127", P=29.33 Y
               9026!); MU=0.67", P=113G; A-SB 2 (MAB-MAA=0.6M,
              P=3.275631D  9025!).
              O-BMOM, BCE TP KOMOHEHTA CCTEM BT-
              C EPEMEHHM TA UV, A COACHO  5716!, TAK-
              E  BY. PBEEH PEE MEHEH CMMAPHO-
              O ECKA CCTEM. CEKTPAHO HAAAC BC-
              KA KOMOHEHTA AB  9025!./PROBABLY ALL THE THREE COM-
              PONENTS OF THE SYSTEM ARE VARIABLES OF THE UV CET
              TYPE, AND ACCORDING TO  5716! ALSO OF THE BY DRA
              TYPE. THE RANGE OF COMBINED BRIGHTNESS OF THE SYSTEM
              IS GIVEN IN THE TABLE. REALLY THE FLARE OF AB COMPO-
              NENT WAS OBSERVED IN THE SPECTROGRAMS  9025!.
V1401  CYG    MIN II 13.6.
V1410  CYG    P>400D.
V1411  CYG    P=1.553478D?
V1412  CYG    MIN II 15.5.
V1414  CYG    CEBEPH KOMOHEHT TECHO AP/NORTHERN COMPO-
              NENT OF A CLOSE PAIR; D=0.04P.
V1416  CYG    MIN II 14.7.
V1417  CYG    MIN II 13.1.
V1421  CYG    B OACT AHETAPHO TMAHHOCT/IN THE REGION
              OF THE PLANETARY NEBULA NGC 6857=K3-50.
V1425  CYG    HA/DEPTH OF MIN II 0.31M.
V1427  CYG    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER M39.
V1429  CYG    MIN II 15.3.
V1430  CYG    MIN II 15.0.
V1436  CYG    MIN II 15.9, D II =0.08P; MIN II - MIN I =0.48P.
V1437  CYG    MIN II 16.0.
V1440  CYG    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6819.
V1465  CYG    OXOA HA ATMEHH./RESEMBLES AN ECLIPSING VA-
              RIABLE.
V1478  CYG    VB A (B 17M:, 3", 80G). KOMAKTH CTOHK PA-
              OEH. HA ACTOTE 5  CTPKTPA POT-
              EHHA C EHTPOM B BEE. BQ  !-BEA C -
              TKOM HPAKPACHOO EH  P T=
              =300GK. OCAHE CEKTPA  7080, 7081, 7523, 9159,
              9160!./COMPACT RADIO SOURCE. EXTENDED STRUCTURE CEN-
              TERED AT THE STAR IS OBSERVED AT 5 GHZ. BQ  ! STAR
              WITH THE EXCESS OF INFRARED RADIATION OF DUST AT T=
              =300GK. DESCRIPTION OF THE SPECTRUM  7080, 7081, 7523,
              9159, 9160!.
V1479  CYG    B OACT TMAHHOCT/IN THE REGION OF THE NEBULA
              IC % ' .
V1481  CYG    MIN II 12.5. B OACT PACCEHHOO CKOEH/IN
              THE REGION OF THE OPEN CLUSTER NGC 7128.
V1485  CYG    ECK B MAX CHO MEHETC./BRIGHTNESS IN MAX
              STRONGLY VARIES.
V1488  CYG    32 CYG. O-BMOM, OPAET EH CCTEM C
              V695 CYG (31 CYG) /PROBABLY ENTERS A COMMON SY-
              STEM WITH V695 CYG (31 CYG).
              0<D<0.011P. P VAR. MIN I =2420670.0+1140.1D*E (J.D.
              2411400-29700). OCE/SINCE J.D.2429700-CM.
              TA./SEE TABLE.
              AHA OXA ATMEH KOMOHEHTA CEKTPAHOO
              KACCA B4 KOMOHEHTOM KACCA K5. HAAETC
              TAKE HEOA ECKA EPEMEHHOCT ECKA
              K-KOMOHEHTA  8896, 9161!. HA ATMEH A-
              BCT OT LAMBDA: 0.04M V, 0.13M B,0.27M (LAMBDA           M
4243A),0.90
              (LAMBDA 3552A)./THE EPOCH OF THE ECLIPSE OF THE B4 TYPE
              COMPONENT BY THE K5 TYPE COMPONENT IS GIVEN. THERE
              IS ALSO SMALL PHYSICAL LIGHT VARIABILITY OF THE K COM-
              PONENT  8896, 9161!. DEPTH OF ECLIPSES DEPENDS OF LAMBDA:
              0.04M V, 0.13M B,0.27M (LAMBDA 4243A),0.90M (LAMBDA
3552A).
V1489  CYG    NML CYG. 17.0M:-18.0M V, B>21M; I-K=+8.17.
              OEH OO HPAKPACH TOK, OCOBEH-
              H HAEM PACPEC AOBO-EBO OO-
              OK. HA OA 2.5"*3.5" BOKP BE - OKOO
              60 CKPETHX CTOHKOB MCC OH  7461!; C-
              TOHK MAEPHOO EH OH, H2O, SIO. ME-
              HEH ECKA EPOH (CM. TAKE  9163!). O'-
              EKT MOET T POTOBEO, HAAEMO B KOH-
              E POECCA KOHEHCA. OH CEKTP, BOMO-
              HO, BOHKAET B PACPEC OOOKE  9165,
              9166!./VERY LARGE IR EXCESS DUE TO EXPANDING GA-
              SEOUS-DUST ENVELOPE. IN THE AREA 2.5"*3.5" AROUND
              THE STAR THE SYSTEM OF ABOUT 60 DISCRETE SOURCES OF
              OH EMISSION IS DETECTED  7461!; SOURCE OF OH, H2O,
              SIO MASER EMISSION. LIGHT VARIATIONS ARE PERIODICAL
              (SEE ALSO  9163!). THE OBJECT MAY BE A PROTOSTAR BEING
              OBSERVED AT THE END OF CONDENSATION PROCESS. THE LATE
              SPECTRUM ARISES PROBABLY IN THE EXTENDING ENVELOPE
               9165, 9166!.
V1490_ V1492  CYG CM./SEE V1479 CYG.
V1493  CYG    CM./SEE V1479 CYG. V1707 CYG 10.5"P.
V1494  CYG    CM./SEE V1479 CYG.
V1495  CYG    B PAOHE TMAHHOCT/IN THE REGION OF THE NEBULA
              NGC 7000.
V1497  CYG    CM./SEE V1495 CYG.
V1498  CYG    CM./SEE V1495 CYG.
V1500  CYG    B TEEHE ABCTA 1983., O HAAA OEH CT-
              POO O'EMA ECKA, ECK HOBO BOPACTA OT 17.6M
              O 13.5M B (J.D.2442632-653.2). OCE MAX HA OT
              MOHOTOHHOE BAHE ECKA HAKABATC KOE-
              AH C AMTO 0.03M-1.0M V; EPO KOEAH
              C J.D.2442656 O J.D.2443100 MEHC B PEE-
              AX 0.1415D  9167, 9168! - 0.137D  9169, 9170!. OCE
              J.D.2443100 MIN=2443696.4827+0.1396133D*E. HEKO-
              TOPE CCEOBATE (CM., HAPMEP,  9173!) CTA-
              T HEOXOMM PHMAT BOEHHOE HAEHE TO-
              O EPOA. EPE MEC OCE MAX ECKA APECT-
              PPOBAHO PAOEHE HA ACTOTAX 2695  8085 M
               9171!./IN AUGUST 1983, BEFORE THE VERY RAPID INCREASE
              OF LIGHT, THE BRIGHTNESS OF THE NOVA GRADUALLY INCREASED
              FROM 17.6M TO 13.5M B (J.D.2442632-653.2). AFTER MAX
              ALMOST MONOTONOUS DECAY OF BRIGHTNESS IS SUPERIMPO-
              SED BY LIGHT VARIATIONS WITH THE AMPLITUDE OF 0.03M-
              1.0M V; THE PERIOD OF THESE VARIATIONS IN THE INTERVAL
              J.D.2442656-43100 CHANGED IN THE RANGE 0.1415D 9167,
              9168! - 0.137D 9169, 9170!.  SINCE J.D.2443100 MIN=
              =2443696.4827+0.1396133D*E. SOME INVESTIGATORS (SEE,
              FOR INSTANCE,  9173!) ADOPT DOUBLE VALUE OF THIS PE-
              RIOD. A MONTH AFTER THE LIGHT MAXIMUM OF THE NOVA THE
              RADIO EMISSION WAS REGISTERED AT 2695 AND 8085 MHZ
               9171!.
V1507  CYG    AHA OXA POKOO MIN I (BEPXHEO COEHEH
              B-KOMOHEHTA); MIN II 7.01, D II =0.20P, MIN II - MIN I =
              =0.29P; E=0.39. HEOHA KPBA ECKA  8213,
              9049!. OPMA KPBO ECKA  H MIN MEHT-
              C. AOBE OTOK  PACPAC OOOKA./
              THE EPOCH OF A BROAD MIN I (SUPERIOR CONJUNCTION OF
              THE B COMPONENT) IS GIVEN; MIN II 7.01; D II =0.20P,
              MIN II - MIN I =0.29P; E=0.39. UNUSUAL LIGHT CURVE
               8213, 9049!. SHAPE OF THE LIGHT CURVE AND DEPTHS OF
              MIN VARY. GASEOUS STREAMS AND EXPANDING ENVELOPE.
V1508  CYG    MIN II 13.3.
V1509  CYG    VB A (B 11.7M, 55", 106G).
V1511  CYG    V-K=13.6M.
V1513  CYG    GLIESE 781; MU ALFA = -0.146S, MU DELTA = -1.00"; SB.
V1515  CYG    B TEMHO TMAHHOCT, B PAOHE TMAHHOCT NGC 6914.
              CBAHA C TMAHHM PATKOM, OXOM HA A-
              T. O'EM ECKA POCXO C 1944 O 1958 .
              C 1958. OCTAETC B MAX. MEEHHE MEHEH
              ECKA C A<=1.6M. B CEKTPE - H OOEH
              LI I LAMBDA 6707 A./IN A DARK NEBULA,  NEAR THE NEBULA
              NGC 6914. CONNECTED WITH NEBULAR APPENDAGE LIKE A
              COMMA. LIGHT INCREASE WAS OBSERVED FROM 1944 TILL
              1958. SINCE 1958 THE STAR IS IN MAX. SLOW LIGHT VARIA-
              TIONS WITH A<=1.6M. THE ABSORPTION LINE LI I LAMBDA 6707A
              IS SEEN IN THE SPECTRUM.
V1521  CYG    CYG X-3. EKPH HPAKPACH CTOHK PEHT-
              EHOBCKOO EH. V>23M. BCXBA PA-
              OCTOHK. B CCTEME K HAATC KOPOTKE
               MEEHHE BCK C XAPAKTEPHM BPEMEHEM
              - 2 MH.  1-2H, HEPABHE MEHEH  O-
              OEPOECKA EPEMEHHOCT  7752!. T ME-
              HEH COPOBOATC EPOECKM KOEAH-
              M HPAKPACHOO, PEHTEHOBCKOO  GAMMA-EH
              C EMEHTAM: MIN=2440949.8986+0.1996830D*E+
              +1.25D*10**-10*E**2  9187!. OHO AMTA TX
              KOEAH A(K)=0.5M, HO HOA OH COBEPEHHO
              CEAT./PECULIAR INFRARED X-RAY SOURCE. V>23M.
              FLARE RADIO SOURCE. IN THE K BAND SHORT AND SLOW FLA-
              RES ON THE TIME SCALE ABOUT 2 MINUTES AND 1-2 HOURS,
              IRREGULAR VARIATIONS AND LONGPERIODIC VARIABILITY ARE
              OBSERVED  7752!. THESE VARIATIONS ARE ACCOMPANIED
              BY PERIODICAL OSCILLATIONS OF INFRARED, X-RAY AND GAMMA
RA-
              DIATION WITH THE ELEMENTS: MIN=2440949.8986+
              +0.1996830D*E+1.25D*10**-10*E**2  9187!. USUALLY THE
              AMPLITUDE OF THESE VARIATIONS A(K)=0.5M, BUT SOME-
              TIMES THEY DISAPPEAR COMPLETELY.
V1523  CYG    AMTA  CPEH BEHA CHO MEHTC./
              AMPLITUDE AND MEAN BRIGHTNESS STRONGLY VARY.
V1531  CYG    LKH ALFA 142. VB A (B=V1532 CYG, 2.5", 90G). CM./SEE
              V1479 CYG. ECK  CEKTP CMMAPHE./COMBINED
              BRIGHTNESS AND SPECTRUM ARE GIVEN.
V1532  CYG    LKH ALFA 143. VB B (A=V1531 CYG; B 2.5", 90G). CM./
              SEE V1531 CYG.
V1535  CYG    CM./SEE V1479 CYG.
V1536  CYG    CM./SEE V1495 CYG.
V1538  CYG    CM./SEE V1495 CYG.
V1539  CYG    CM./SEE V1495 CYG.
V1540  CYG    CM./SEE V1495 CYG.
V1546  CYG    CM./SEE V1495 CYG.
V1548  CYG    VB A (B 16.7M, 6.2", 131G).
V1554  CYG    VB A (B 14.7M, 3.5", 214G).
V1577  CYG    B CKOEH  TMAHHOCT/IN THE CLUSTER AND NEBULA
              IC 5146.
V1578  CYG    CM./SEE V1577 CYG. VB A (B 15M, 5", 45G; C 17M,
              5", 225G). CBAHA C OTPAATEHO TMAHHOCT./
              ASSOCIATED WITH A REFLECTING NEBULA.
V1580  CYG    EMEHT COEPAT CHCOAH EH:/THERE
              IS A PERIODIC TERM IN THE ELEMENTS:-0.027D SIN 0.045G
              (J.D.-2439000).
V1581  CYG    G 208-44. VB A (B=G 208-45, 15.97M V, M6VE; 7.9",
              106G, 1954; 8.2", 96G, 1974). MU=0.71", P=140G. BC-
              KA HAAAC P CEKTPAHX HAEHX
               9175!. CTHK TAKE MOET T EPEMEHHO TA
              UV CET. AH PEE MEHEH CMMAPHOO EC-
              KA CCTEM./THE FLARE WAS OBSERVED DURING SPECTRO-
              SCOPIC OBSERVATIONS  9175!. THE COMPANION MAY BE
              ALSO A UV CET TYPE VARIABLE. THE RANGE OF COMBINED
              BRIGHTNESS VARIATION OF THE SYSTEM IS GIVEN.
V1584  CYG    AHA OXA MIN ECKA./EPOCH OF MIN BRIGHTNESS IS
              GIVEN.
V1597  CYG    CM./SEE V1479 CYG.
V1598  CYG    CM./SEE V1479 CYG.
V1600  CYG    CM./SEE V1479 CYG.
V1608  CYG    CM./SEE V1495 CYG.
V1610  CYG    HPAKPACH CTOHK CRL 2688, BEA CEKT-
              PAHOO KACCA F51A, ACCOPOBAHHA C OP-
              HO OTPAAE TMAHHOCT (TMAHHOCT O).
              CEBEPH KOMOHEHT TMAHHOCT HAXOTC B 4" K
              CEBEP OT CTOHKA. C 1920 O 1958. HTEPA-
              H ECK CEBEPHOO KOMOHEHTA BOPOC OT 15.2M
              O 13.4M B  C TEX OP OCTAETC OCTOHHM  8735!.
              ECK CAOO (16.2M B) HOO KOMOHEHTA, HAXO-
              EOC B 5" K  OT CTOHKA, MEHETC HA
              0.6M B  9176!. EHE CHO OPOBAHO (46%,
              TETA=106G B CCTEME V). B CEKTPE - H OOE-
              H C3, MCC NA, C2,  S II!. BOMOHO, BOHKA-
              A AHETAPHA TMAHHOCT  9178!./INFRARED SOURCE
              CRL 2688, THE STAR OF THE SPECTRAL TYPE F51A, ASSOCIA-
              TED WITH A BIPOLAR REFLECTION NEBULA (THE SO-CALLED EGG
              NEBULA). THE NORTHERN COMPONENT OF THE NEBULA IS 4"
              TO THE NORTH FROM THE SOURCE. SINCE 1920 TO 1958 THE
              INTEGRATED LIGHT OF THIS COMPONENT INCREASED FROM 15.2M
              TO 13.4M B AND AFTER THAT DOES NOT VARY  8735!. LIGHT
              OF THE FAINT (16.2M B) SOUTHERN COMPONENT (5" TO THE
              SOUTH FROM THE SOURCE) VARIES BY 0.6M B  9176!. THE
              RADIATION OF THE NEBULA IS STRONGLY POLARIZED (46%,
              TETA=106G IN V SYSTEM). THERE ARE C3 ABSORPTION FEA-
              TURES AS WELL AS NA, C2, AND  S II! EMISSION IN THE
              SPECTRUM. PROBABLY THE OBJECT IS A PRECURSOR OF A PLA-
              NETARY NEBULA  9178!.
V1611  CYG    CM./SEE V1495 CYG.
V1624  CYG    A VAR. B 1957.  BE CEKTPAHOO KACCA B
              PEBPATAC B BE KACCA BE. BOMOHO, OTHO-
              CTC TAKE K T GCAS./IN 1957 OUT OF A B STAR
              TURNED INTO BE STAR. PROBABLY MUST BE REFERRED ALSO
              TO GCAS TYPE.
V1661  CYG    VB A (B 11.14M, 20", 174G).
V1668  CYG    HA HCXOE BETB KPBO ECKA OCE J.D.
              2443765 OHAPEH CHCOAHE KOEAH
              ECKA C A(V)=0.15M  EMEHTAM: MIN=
              =2443767.475+0.4392D*E  9179!. HPAKPACHE KP-
              BE ECKA (1.6-10 MKM) MET BTOPH MAKC-
              MM (J.D.2443815), CBAHH C OPAOBAHEM -
              EBO OOOK. HA 10 MKM TOT BTOPH MAKC-
              MM PE ABHOO  9069!./THERE ARE SINUSOIDAL
              LIGHT VARIATIONS WITH A(V)=0.15M AND ELEMENTS MIN=
              =2443767.475+0.4392D*E IN THE DESCENDING BRANCH
              OF THE LIGHT CURVE AFTER J.D.2443765  9179!. INFRARED
              LIGHT CURVES (1.6-10 MU M) HAVE A SECONDARY MAXIMUM (J.D.
              2443815) DUE TO THE FORMATION OF THE DUST ENVELOPE.
              AT 10 MU M THIS SECONDARY MAXIMUM IS BRIGHTER THAN THE
              PRIMARY ONE  9069!.
V1669  CYG    D=0.036P.
V1671  CYG    DU=0.06.
V1674  CYG    VB (B 15M, 5"). AH PEE MEHEH CMMAP-
              HOO ECKA. HE CKEHO, TO EPEMEHHM B-
              ETC KOMOHEHT B. HA MEEHHE MEHEH CPE-
              HEO ECKA B PEEAX 10.555M-10.570M B HAKA-
              BATC CHCOAHE EPOECKE C P1=1.3608D
              (A1=0.0037M)  P2=0.8055D (A2=0.0032M)./THE RANGE
              OF COMBINED BRIGHTNESS VARIATION IS GIVEN. IT IS NOT
              EXCLUDED THAT IT IS THE COMPONENT B THAT IS VARIABLE.
              SLOW VARIATIONS OF MEAN BRIGHTNESS IN THE RANGE
              10.555M-10.570M B ARE SUPERIMPOSED BY SINUSOIDAL PE-
              RIODIKAL ONES WITH P1=1.3608D (A1=0.0037M) AND P2=
              =0.8055D (A2=0.0032M).
V1676  CYG    B PACCEHHOM CKOEH/IN THE OPEN CLUSTER NGC 6871.
              ADS 13374 A (B 12.0M, 6.5", 64G; C 11.0M, 9.5", 28G;
              D9.5M, B3V, 11.4", 301G; E 11.42M, 28.1", 109G; F 7.36M,
              B 1IA, 35.9", 29G); SB2 (P=112.7D).
V1696  CYG    SB 1 (PORB=4.3174D). AHA OXA MIN ECKA. BOMO-
              HO ATMEHE AKKPEOHHOO CKA, OKPAEO KOM-
              AKTH O'EKT, OPAOBABC P BCKE CBEPX-
              HOBO B BOHO CCTEME -5*10**6 ET HAA  3619!./
              EPOCH OF MIN BRIGHTNESS IS GIVEN. THE ECLIPSE OF THE
              ACCRETION DISC AROUND THE COMPACT OBJECT FORMED IN
              THE OUTBURST OF A SUPERNOVA IN A BINARY SYSTEM ABOUT
              5*10**6 YEARS AGO IS POSSIBLE  3619!.
V1701_ V1704  CYG CM./SEE V1479 CYG.
V1706  CYG    CM./SEE V1479 CYG.
V1707  CYG    CM./SEE V1479 CYG. V1493 CYG 10.5"F.
V1711  CYG    CM./SEE V1495 CYG.
V1716  CYG    CM./SEE V1495 CYG.
V1719  CYG    OPMA KPBO ECKA MEHETC./SHAPE OF THE LIGHT
              CURVE VARIES.
V1720  CYG    MIN II 7.79.
V1721  CYG    P VAR.MIN I=2442605.497+2.724370D*E (J.D.2442311-
              928); OCE/SINCE J.D.2442928-CM.TA./SEE
              TABLE.
V1722  CYG    MIN II 14.6?
V1726  CYG    BOMOH EH EMHHOO PACCEHHOO CKOE-
              H/POSSIBLE MEMBER OF AN ANONIMOUS OPEN CLUSTER.
V1727  CYG    4U 2129+47. LX/LOPT-10. MCC B CEKTPE:/
              EMISSIONS IN THE SPECTRUM: NEII LAMBDA 4686A, CIII-NIII
              LAMBDA LAMBDA 4640-50A.
V1735  CYG    B KOMEKCE TEMHX TMAHHOCTE, ACCOPOBAH-
              HX C PACCEHHM CKOEHEM  TMAHHOCT
              IC 5146. OCBEAET OTPAATEH TMAHHOCT.
              CTAA PE O KPAHE MEPE HA 5M C 1952 O 1965./
              IN THE COMPLEX OF DARK NEBULAE ASSOCIATED WITH THE
              OPEN CLUSTER AND THE NEBULA IC 5146. LIGHTS UP A
              REFLECTING NEBULA. BECAME BRIGHTER DY 5M AT LEAST
              FROM 1952TO 1965.
V1737  CYG    B-V=+3.7.
V1738  CYG    B-V=+5.5:.
V1739  CYG    B-V=+4.5:.
V1744  CYG    PBEEHA OXA MAX B CCTEME U./EPOCH OF MAX
              IN U SYSTEM IS GIVEN.
V1746  CYG    HOA HAAETC P=0.21D./SOMETIMES P=0.21D
              IS OBSERVED.
V1747  CYG    P>100D. B-V=+4.0.
V1748  CYG    B TMAHHOCT/IN THE NEBULA IC 1318A.
V1751  CYG    B TMAHHOCT/IN THE NEBULA IC 1318C.
V1761  CYG    BOMOHO HAE TECHOO CTHKA. EMEHT HE-
              BEPEHHE./CLOSE COMPANION? ELEMENTS ARE NOT
              CERTAIN.
ALFA   CYG    VB A (B 11.4M, 75.3", 106G).
R      CYG    VB A (B 6.44M, G1V, A=0.88", P=49.80YR; C 12.20M,
              29", 230G). 0.083D<=P<=0.125D. AH PEE ME-
              HEH CMMAPHOO ECKA./THE RANGE OF TOTAL LIGHT
              VARIATION IS GIYEN.
IPSILO CYG    VB A (B 10.2M, 15.2", 220G; C 10.2M, 21.5", 180G).
HI     CYG    VB A (B 10.8M, 158", 254G). S 6+%1E (TC). SIO MAEP/
              MASER. P VAR.MAX=2393559+405.88D*E (J.D.
              2337150-94000); OCE/SINCE J.D.2394000-CM.
              TA./SEE TABLE.
P      CYG    OBEHE BE BEPBE OTMEEHO B 1600., KO-
              A EE ECK  3M. C XVIII CTOET ECK BE-
               MEHETC B HTEPBAE 4.6M-5.6M VIS. PAOC-
              TOHK B MMETPOBOM  CAHTMETPOBOM AAO-
              HAX/THE APPEARANCE OF THE STAR WAS FIRSTLY NOTED IN
              1600, WHEN ITS BRIGHTNESS WAS 3M. SINCE THE XVIII
              CENTURY THE LIGHT OF THE STAR VARIES IN THE RANGE 4.6M-
              5.6M VIS. RADIO SOURCE AT THE MILLIMETRE AND CENTI-
              METRE WAVELENGTHS.
Q      CYG    B MHMME ECK MEHETC EPOECK C AM-
              TO 0.5M: MAX=2440495+54.99D*E; BOMOEH TAK-
              E P=64.81D. CPEH POBEH ECKA MEHETC B
              PEEAX 15.2M-15.9M B./IN MINIMUM BRIGHTNESS VARIES
              PERIODICALLY WITH THE AMPLITUDE 0.5M: MAX=2440495+
              +54.99D*E; P=64.81D IS ALSO POSSIBLE. MEAN LEVEL OF
              BRIGHTNESS VARIES IN THE RANGE 15.2M-15.9M B.
S      DEL    VB A (B 56", 342G).
              HOA HAATC BOHE MAKCMM./DOUBLE
              MAXIMA ARE SOMETIMES OBSERVED.
U      DEL    CPEH ECK/MEAN BRIGHTNESS VAR, P=1100D.
              COACHO  8993!, OEE BEPOTEH EPO 160D-180D,
              EM 110D./ACCORDING TO  8993!, THE PERIOD VALUE 160D-
              180D IS MORE LIKELY THAN 110D.
W      DEL    D=0.017P. MIN II 9.79. P VAR. OCE/SINCE J.D.
              2433000-CM.TA./SEE TABLE.
              OPMA KPBO ECKA./THE LIGHT CURVE SHAPE VAR.
RZ     DEL    VB (A VAR; B VAR, 17", 137G)  3771!.
TT     DEL    P VAR. OCE/SINCE J.D.2435000-CM.TA./SEE
              TABLE.
TW     DEL    DM VAR (0.5M+3.4M).
              KPBA ECKA HAOMHAET RV TAU, C MIN I  MIN II;
              AHA OXA MIN I./THE LIGHT CURVE RESEMBLES THAT OF
              RV TAU, WITH MIN I AND MIN II; THE EPOCH OF MIN I IS
              GIVEN.
              MIN I=2432171.1+118.4D*E (1947-1952); MIN I=
              =2435386.8+115.9D*E (1955-1963); B HTEPBAE/DURING
              1964-1970-CM.TA./SEE TABLE.
TX     DEL    P VAR. P=6.166585D (J.D.2428000-36600); OCE/SINCE
              J.D.2436600-CM.TA./SEE TABLE.
TY     DEL    MIN II 9.8. P VAR.MIN=2428020.399+1.191121D*E (J.D.
              2428000-38000)  0279!; OCE/SINCE J.D.2438000-CM.
              TA./SEE TABLE.
TZ     DEL    AHA OXA MIN./EPOCH OF MIN IS GIVEN.
VV     DEL    HA/DEPTH OF MIN II 0.05M.
YY     DEL    BOMOEH MIN II HO-0.05M./MIN II OF THE DERTH
              -0.05M IS POSSIBLE.
              P VAR. MIN=2425795.488+0.7930856D*E (J.D.2425000-
              34000)  1329!; OCE/SINCE J.D.2434000-CM.TA./
              SEE TABLE.
AL     DEL    MIN II 12.4.
BG     DEL    MIN II 13.8.
BK     DEL    P VAR?
BR     DEL    OH MCC/EMISSION.
BX     DEL    DS=0.
BY     DEL    MIN II 11.8.
CE     DEL     FE/H!=-0.68.
CF     DEL    OPMA KPBO ECKA/THE LIGHT CURVE SHAPE VAR?
CH     DEL     FE/H!=-1.23.
              COACHO/ACCORDING TO  9037!, P=0.315D.
CN     DEL    MIN II 14.6.
CR     DEL    MIN II 13.7.
CS     DEL     FE/H!=-0.92.
CU     DEL    OTMEAETC CKAKOOPAHOE MEHEHE A./
              ABRUPT PHASE CHANDE WAS NOTED.
CW     DEL    P VAR.P=0.58209D (J.D.-2427100), P=0.58211D (J.D.
              -2428800); B HTEPBAE/DURING J.D.2429800-30600-
              CM.TA./SEE TABLE.
DG     DEL    EMEHT HATC B POBEPKE./THE ELEMENTS
              SHOULD BE CHECKED.
DK     DEL    MIN II 14.2.
DM     DEL    MIN II 8.80.
DT     DEL    AHA OXA MIN. EMEHT CPABEB B HTEPBA-
              E J.D.2425480-6260./EPOCH OD MIN IS GIVEN. THE
              ELEMENTS ARE VALID DURING J.D.2425480-6260.
DX     DEL     FE/H!=-0.11.
EG     DEL    P VAR. MAX=2425535.42+0.3248545D*E (J.D.2425478-
              30619)  0911!; MEHEHE CKAKOM OKOO J.D.
              2432578, AEE CM.TA./ABRUPT CHANGE NEAR J.D.
              2432578, SINCE THEN SEE TABLE.
EL     DEL    CPEH BEHA/THE MEAN BRIGHTNESS VAR, P-600D.
EK     DEL    B-V: +0.29, +0.53.
ES     DEL    OX MAX   3715!,  7527! POTBOPEAT PBEEH-
              HM EMEHTAM./EPOCH OF MAX FROM  3715!,  7527!
              CONTRADICT THE GIVEN ELEMENTS.
ET     DEL    MIN II 12.7.
EW     DEL    MIN II 15.5.
EX     DEL    MIN II 13.3.
FL     DEL    MIN II 14.5.
FK     DEL    MIN II 14.5.
FM     DEL    DS=0.
FP     DEL     FE/H!=-1.44.
FR     DEL    MIN II 15.3.
FT     DEL    EKT AKO?/BLAZHKO EFFECT?
GG     DEL    MIN II 12.6. P VAR?
GN     DEL    P VAR? DM VAR?
GY     DEL    VB B (A=BD+15G4134A, SP A-F).
HR     DEL    PORB=0.170920D.
              ECK HAA PACT B J.D.-2439653. BOH C MAKC-
              MMAM J.D.2439752 (4.55M), 2439799 (4.64M), ATEM
              OCTP ABH MAX, OCK MAX J.D.2439981 (4.09M)
               AEHE ECKA. PAOCTOHK./THE BRIGHTNESS
              BEGAN TO INCREASE ON J.D.-2439653. WAVES WITH MA-
              XIMA ON J.D.2439752 (4.55M), 2439799 (4.64M), FOLLOWED
              DY A SHARP MAIN MAX, FLAT MAX ON J.D.2439981 (4.09M)
              AND FINAL DECLINE. RADIO SOURCE.
HU     DEL    MU=0.685", TETA=79G.
              ACTPOMETPECKA BOHA/ASTROMETRIC BINARY (O-
              AMTA OTKOHEH/SEMIAMPLITUDE OF DEVIATIONS
              0.118", PORB=1.52YR).
II     DEL     FE/H!=-1.30.
IO     DEL    HAAAC TOKO OHA BCKA/A SINGLE OUTBURST
              WAS OBSERVED (J.D.2439378-388).
IV     DEL    D-0.1D.
LS     DEL    MIN II 8.76.
DELTA  DEL    (K-B)2=0.19. SB 2 (PORB=40.58D; E=0.7).
              CEKTP OOX KOMOHEHTOB SB OKABAT AM-XA-
              PAKTEPCTK; ET FE, CA, SC, TOK SR, Y,
              ZR, BA, CE, LA, EU. OA KOMOHEHTA-EPEMEHHE
              TA DSCT; EPO CA ABHOO KOMOHEH-
              TA 0.158D, CTHKA-0.134D  7528!. KAOE  KOE-
              AH BPEMEHAM OMHPET B CMMAPHOM ECKE:
              COACHO  7529!, MAX=2439338.4444+0.135547D*E;
              COACHO 7530!, P=0.154991D./SPECTRA OF BOTH SB
              COMPONENTS SHOW AM FEATURES; FE, CA, SC DEFICIEN-
              CY, SR, Y, ZR, BA, CE, LA, EU EXCESS. BOTH COMPO-
              NENTS ARE DSCT VARIABLES; THE PERIOD OF THE MAIN COM-
              PONENT PULSATION IS 0.158D, THAT OF THE SECONDARY IS
              0.134D  7528!. ANY OF THE OSCILLATIONS MAY OCCASIO-
              NALLY DOMINANTE IN THE COMBINED BRIGHTNESS: ACCORDING
              TO 7529!, MAX=2439338.4444+0.135547D*E; ACCOR-
              DING TO  7530!, P=0.154991D.
R      DOR    VB A (B 11.9M, 34", 10G; C 11.0M, 35", 130G, 1933).
              H2O, SIO, HC3N MCC/EMISSION.
S      DOR    VB A (B 12.1M, 13"). EH OOO MAEAHOBA
              OAKA. B CKOEH NGC 1910  HO TMAH-
              HOCT. OHA  HAOEE PKX O ACOTHO BE-
              HE BE. OKE MIN: 1891, 1900, 1930, 1940,
              1955, 1964./THE MEMBER OF THE LARGE MAGELLANIC
              CLOUD. IN THE CLUSTER NGC 1910 AND A DIFFUSE NEBULA.
              ONE OF THE ABSOLUTELY BRIGHTEST STARS. DEEP MIN: 1891,
              1900, 1930, 1940, 1955, 1964.
T      DOR    VB A (B 12.0M VIS, 5", 13G).
V      DOR    HA PAHE OOO MAEAHOBA OAKA./AT THE
              EDGE OF THE LARGE MAGELLANIC CLOUD.
W      DOR    B OACT OOO MAEAHOBA OAKA./IN THE
              REGION OF THE LARGE MAGELLANIC CLOUD.
X-Y    DOR    EH  OOO MAEAHOBA OAKA./THE MEMBER
              OF THE LARGE MAGELLANIC CLOUD.
Z      DOR    CM./SEE X DOR. B TMAHHOCT/IN THE NEBULA 30 DOR.
RR     DOR    CM./SEE W DOR. MIN II 14.5.
RS     DOR    CM./SEE W DOR.
RU     DOR    CM./SEE X DOR.
RW     DOR    CM./SEE SW DOR. MIN II 11.2.
RX     DOR    CM./SEE W DOR. HE EH OAKA?/CLOUD NON-MEMBER?
RY     DOR    CM./SEE X DOR.
SW     DOR    B OACT OOO MAEAHOBA OAKA, HE EH
              OAKA./IN THE REGION OF THE LARGE MAGELLANIC CLOUD.
              CLOUD NON-MEMBER.
              P VAR  9036!.
SX     DOR    B OACT OOO MAEAHOBA OAKA, HE EH
              OAKA./IN THE REGION OF THE LARGE MAGELLANIC CLOUD,
              CLOUD NON-MEMBER.
              DM VAR.
SY     DOR    CM./SEE W DOR. COACHO  9036!, EPEMEHHOCT COM-
              HTEHA./ACCORDING TO  9036!, VARIABILITY IS DOUBT-
              FUL.
SZ     DOR    B OACT OOO MAEAHOBA OAKA, HE EH
              OAKA./IN THE REGION OF LARGE MAGELLANIC CLOUD,
              CLOUD NON-MEMBER.
TT_TW  DOR    CM./SEE W DOR.
TX     DOR    CM./SEE X DOR.
TY     DOR    CM./SEE SZ DOR.
TZ     DOR    CM./SEE X DOR.
UU_UV  DOR    CM./SEE SZ DOR.
UW     DOR    CM./SEE W DOR.
UX     DOR    CM./SEE SZ DOR.
UZ_VV  DOR    EH OOO MAEAHOBA OAKA?/THE LARGE
              MAGELLANIC CLOUD MEMBER?
XX     DOR    CM./SEE SZ DOR.  FE/H!--1.3.
ZZ     DOR    CM./SEE SZ DOR.
AA     DOR    D=0.02P. MIN II 11.21.
ALFA   DOR    VB A (B 4.3M, A=0.2125", P=13.00YR.)
              AH PEE MEHEH CMMAPHOO ECKA./THE
              RANGE OF COMBINED BRIGHTNESS VARIATIONS IS GIVEN.
BETA   DOR    P VAR. AH TEKE EMEHT./CURRENT ELEMENTS
              ARE GIVEN.
T      DRA    ADS 10937 A (B=UY DRA, OTECK/OPTICAL, 16",
              222G).
U      DRA    P VAR. AH CPEHE EMEHT./MEAN ELEMENTS ARE
              GIVEN.
W      DRA    P VAR. MAX=2416748+257.11D*E (J.D.2416750-
              21390); MAX=2430826+262.11D*E (J.D.2421390-
              30820); MAX=2439962+268.87D*E (J.D.2430820-
              40490); OCE/SINCE J.D.2440490-CM.TA./SEE
              TABLE.
Y      DRA    O BAHM HAEHM/ACCORDING TO VISUAL
              OBSERVATIONS, 7.8M-15.0M.
Z      DRA    MIN II 11.0. P VAR. MIN=2430973.314+1.3574176D*E
              (J.D.2428460-33300); MIN=2433268.708+
              +1.357440D*E (J.D.2433300-43500); OCE/SINCE J.D.
              2443500-CM.TA./SEE TABLE.
RR     DRA    D=0.015P. MIN II 10.1. P VAR.
              O/BEFORE J.D.2439000 MIN I=2433390.458+
              +2.83123D*E  1001!; OCE/SINCE J.D.2440000-CM.
              TA./SEE TABLE.
RS     DRA    AH CPEHE EMEHT/MEAN ELEMENTS ARE GIVEN
              (J.D.2415120-37584); B HTEPBAE/DURING J.D.
              2436012-37584 P=145.3D.
              DM  OPMA KPBO ECKA CHO MEHTC./DM
              AND THE LIGHT CURVE SHARE VARY STRONGLY.
RW     DRA    P VAR. AH TEKE EMEHT./MEAN ELEMENTS ARE
              GIVEN.
              COH EKT AKO:/COMPOSITE BLAZHKO EFFECT;
              =93.95P=41.61D; 1=280P; 2=6140P; 3=
              =3400P  1585!. 0.11P<=M-M<=0.32P. DS=3.
RX     DRA    MIN II 10.3, D II=0.009P.
RZ     DRA    MIN II 10.38. P VAR. MIN=2429448.787+0.55087668D*E
              (1907-1968)  3822!; OCE/SINCE 1968-CM.TA./
              SEE TABLE.
SU     DRA    P VAR. O/BEFORE 1955 MAX HEL=2420605.762+
              +0.66041890D; OCE/SINCE 1955-CM.TA./SEE
              TABLE.  FE/H!=-1.39.
SW     DRA    DS=3.5.
SX     DRA    D=0.035P. MIN II 10.0. P VAR. MIN I=2432273.276+
              +5.1692D*E (J.D.2432000-38000); OCE/SINCE J.D.
              2442000-CM.TA./SEE TABLE.
TT     DRA    P2=198D.
TW     DRA    ADS 9706 A (B 9.5M VIS, 23G, 3.6"). D=0.02P; MIN II 8.1.
              P VAR. MIN I=2433888.452+2.806870D*E (J.D.
              2433000-40000)  3825!; OCE/SINCE J.D.2440000-
              CPEHE EMEHT B TAE./MEAN ELEMENTS IN THE
              TABLE.
TX     DRA    CPEH BEHA/MEAN MAGNITUDE VAR, P2=654D.
UU     DRA    CPEH BEHA/MEAN MAGNITUDE VAR, P2=960D.
UX     DRA    COACHO  9086!, O KPBO ECKA BOMOEH T E;/
              ACCORDING TO  9086!, THE LIGHT CURVE MAY CORRESPOND
              TO THE TYPE E;SB, P-340D.
UZ     DRA    D=0.01P; MIN II 10.6. BOMOHO, /POSSIBLY P=1.65D
               3827!.
VW     DRA    O OTOEKTPECKM AHHM/ACCORDING TO PHOTO-
              ELECTRIC OBSERVATIONS, 6.28M-6.32M V.
VX     DRA    BOMOEH T E/TYPE E IS POSSIBLE, P=0.892D/N.
WW     DRA    KBAPATH EH:/NONLINEAR TERM:-4.98D*10**-9*E2.
              ADS 10152A (B 9.67M, 8.2", 5G).
              HA/DEPTH OF MIN II 0.08M.
WZ     DRA    DM VAR CHO/STRONGLY.
XY     DRA    MIN II 13.7.
XZ     DRA    P VAR. O/BEFORE J.D.2438000 MAX=2427985.648+
              +0.4764944D*E  0188!.
              OX OCE J.D.2438000 EMEHTAM B TAE
              PECTABTC  B CPEHEM. EKT AKO;
              COACHO  1474!, =78D./EPOCHS AFTER J.D.2438000
              ARE REPRESENTED DY THE ELEMENTS IN THE TABLE ONLY ON
              AVERAGE. BLAZHKO EFFECT; ACCORDING TO  1474!, =78D.
               FE/H!=-0.57.
ZZ     DRA    P VAR. MAX=2434509+274.5D*E (J.D.2416350-
              34600); OCE/SINCE J.D.2437100-CM.TA./SEE
              TABLE.
AE     DRA    DS=(4).
AF     DRA    VR VAR; SB?
AG     DRA    CTOHK MKOO PEHTEHOBCKOO EH. E-
              MEHT B TAE OCBAT OX MAX B AX U
              B 1974-1979  9113!./A SOFT X-RAY SOURCE. ELEMENTS
              IN THE TABLE REPRESENT MAXIMA IN U BAND IN 1974-
              1979  9113!.
AI     DRA    MIN II 7.16, D II=0.17P.
AP     DRA    BOMOEH BBOE MEH EPO./TWICE SHORTER PE-
              RIOD IS POSSIBLE.
AQ     DRA    CEKTPAHA H H BETA, BOMOHO, AOHEHA
              MCCE./H BETA SPECTRAL LINE IS PROBABLY FILLED IN DY
              EMISSION.
AR     DRA    MIN II 11.63.
AS     DRA    MU=0.486", P=289G. SB. DM VAR. OA POCTPAH-
              CTBEHHA CKOPOCT./LARGE SPATIAL VELOCITY.
              ECK MEHETC B ABCMOCT OT A OPTA-
              HOO BEH. A MAX  MIN B PAHX KAX
              PAH. B TAE PBEEH PORB  3075!  O-
              XA COEHEH (G4-BEA CA)./THE BRIGHTNESS
              VARIES WITH THE PHASE OF THE ORBITAL MOTION. PHASES
              OF MAX AND MIN VARY FROM CYCLE TO CYCLE. THE TABLE
              GIVES PORB 3075! AND THE EPOCH OF THE CONJUNCTION
              (G4-STAR IS BEHIND).
AW     DRA    P VAR. OCE/SINCE J.D.2430500-CM.TA./SEE
              TABLE.
AX     DRA    MIN II 11.0.
BE     DRA    MIN II 11.5. CEKTPAH KACC-OH B./THE
              SPECTRAL TYPE IS LATE B.
BH     DRA    ADS 12019A (B AM, 9.25M, 10.8", 58G). MIN II 8.58.
BK     DRA    P VAR.MAX=2415150.817+0.592019D*E (J.D.
              2414900-16150)  0001!; OCE/SINCE J.D.2416940-
              CM.TA./SEE TABLE.
              DS=8 B MAX ECKA/IN MAX LIGHT.
BP     DRA    MIN II 14.7.
BS     DRA    MIN II 9.84.
BV     DRA    ADS 9537 A (B=BW DRA, 16.3", 358G, 1980; C 12.69M).
              MIN II 8.40.
BW     DRA    ADS 9537 B (A=BV DRA; C 12.69M). MIN II 9.02.
BY     DRA    SB 2 (PORB=5.9750998D, E=0.36). MU=0.365", P=150G.
              KBAEPOECKA EPEMEHHOCT: DM VAR, P VAR
              (EPEHAHOE BPAEHE/DIFFERENTIAL ROTATION),
              CKAK A/PHASE JUMPS. BCK O DU=1.07M./
              FLARES UP TO DU=1.07M.
CM     DRA    VB A (B SP=DC, 15.7M PG, 25.7", 22G, OEE/COM-
              MON MU). MU=1.619", P=317G, PI=0.068", VNU=-118.6KM/S.
              MIN II 13.63. EPEMEHHOCT TA BY:/BY TYPE VA-
              RIABILITY: DM<=0.05MV, P-PORB. BCK:/FLARES:
              DM-0.05M.
CR     DRA    MU=0.50", P=168G, PI=0.048".
CX     DRA    SB, PORB=6.69612D (C TM EPOOM/WITH THIS PE-
              RIOD DV=0.04M).
              MEEHHE KECKE MEHEH:/LONG-TERM
              CYCLIC VARIATIONS: P-2400D, DV-0.2M.
              BCK/FLARES-0.1M.
              PEHTEHOBCK CTOHK:HAAETC EKT OT-
              PAEH./AN X-RAY SOURCE; THE REFLECTION EFFECT IS
              OBSERVED.
DE     DRA    D=0.017P.
DG     DRA    H OTHOCTEHO/DEPTHS RESPECTIVE TO MAX I
              (=0.25); MIN II 0.17M; MAX II 0.01M.
DK     DRA    PORB=64.44D. AHA OXA MIN. MCC H  KCA II
               OOX KOMOHEHTOB./EPOCH OF MIN IS GIVEN. BOTH
              COMPONENTS SHOW H AND K CAII IN EMISSION.
DL     DRA    VB A (B 9.2M, 3.9", 318G, 1982). P1=0.0825D, A1=
              =0.028M;P2=0.0837D, A2=0.026M.
DN     DRA    P=109S. MU=0.32", P=153G.
K      DRA    K TOK/IR EXCESS.
      DRA    ADS 11311 (DM=1.7M, 0.3", 288G, 1967). A:SB, P=
              =26.768D. AHA OXA MAX B AX U./THE EPOCH OF
              MAX U LIGHT IS GIVEN.
S      EQU    MIN II 8.11. P VAR. O/BEFORE J.D.2427000 MIN=
              =2423746.490+3.4360050D*E  1140!; MIN=
              =2437968.345+3.436072D*E (J.D.2427000-41000)
               3432!; OCE/SINCE J.D.2441000-CM.TA./SEE
              TABLE.
              AOBE OTOK; B MIN ECKA H ALFA B MCC./
              GASEOUS STREAMS; IN MIN LIGHT H ALFA IS IN EMISSION.
W      EQU    MIN II 12.4. P VAR.
Z      EQU    KA BEA:/A NEARBY STAR: 12.1M.
RT     EQU    P VAR CHO./STRONGLY.
RW     EQU    CH EKT AKO./STRONG BLAZHKO EFFECT.
RZ     EQU    MIN II 12.2:.
SU     EQU    MIN II 16.4.
SV     EQU    HA/DEPTH OF MIN II 0.16M.
SW     EQU    MIN II 15.6.
NU     EQU    ADS 14702A (B 11.6M, 2", 268G; C 12.6M, 48", OT-
              ECK/OPTICAL). B TAE AH EPO OC.
              CBEEH O EPOHOCT BPAATEHO EPEMEH-
              HOCT ECKA, CEKTPA  MAHTHOO O POTBO-
              PEB (17.492D, 314D, 1785.7D, 72YR)./THE TABLE
              GIVES THE PERIOD OF OSCILLATIONS. DATA ON THE PERIO-
              DICITY OF THE ROTATIONAL VARIABILITY OF LIGHT, SPECTRUM
              AND MAGNETIC FIELD ARE CONTRADICTORY (17.492D, 314D,
              1785.7D, 72YR).
V      ERI    CPEH BEHA/MEAN MAGNITUDE VAR, P2=1209D.
W      ERI    SIO, OH, H2O MAEP/MASER.
Z      ERI    P2=746.4D.
RU     ERI    MIN II 9.62.
RX     ERI     FE/H!=-1.32.
RY     ERI    D=0.025P.
RZ     ERI    D=0.018P. HA/THE DEPTH OF MIN II 0.04M PG.
SV     ERI     FE/H!=-1.83. P VAR. P=0.71365272D (J.D.2414000-
              21000); P=0.71370172D (J.D.2421000-26000)  0862!;
              MAX=2426590.319+0.7137406D*E (J.D.2426000-
              34000)  9195!; OCE/SINCE J.D.2434000-CM.TA./
              SEE TABLE.
TT     ERI    (B-V)MAX=+0.255M.
TV     ERI    (B-V)MAX=+0.53M.
TZ     ERI    D=0.015P. P VAR. MIN=2426066.198+2.606097D*E (J.D.
              2426000-33500)  1490!; OCE/SINCE J.D.2438200-
              CM.TA./SEE TABLE.
UX     ERI    MIN II 11.01. P VAR? O/BEFORE J.D.2438500 MIN I=
              =2434368.570+0.4452820D  2494!; OCE/SINCE J.D.
              2438500-CM.TA./SEE TABLE.
UY     ERI    OPMA KPBO ECKA/THE SHAPE OF THE LIGHT CURVE
              VAR.  A/H!=-1.6.
VW     ERI    BA EPOA CMEHT P PA:/ALTERNATING P1=
              83.4D, P2=93.3D.
              HACEEHE AO./HALO POPULATION.
WW     ERI    MIN II 11.2.
WX     ERI    HA/THE DEPTH OF MIN II 0.22M.
              ABH KOMOHEHT/THE PRIMARY COMPONENT VAR,
              DSCT:,  P1=0.16454D, P2=0.13721D.
YY     ERI    MIN II 8.72. P VAR. MIN I=2433617.5198+0.321496212D*E
              (J.D.2433000-41500)  3850!; OCE/SINCE 2441500-
              CM.TA./SEE TABLE.
              PEHTEHOBCK CTOHK./X-RAY SOURCE.
ZZ     ERI    MIN II 14.4.
AN     ERI    MIN II 14.9.
AO     ERI    D=0.04P.
AS     ERI    MIN II 8.42. PEHTEHOBCK CTOHK./X-RAY SOURCE.
BB     ERI    (K-D)2=0.13.
BC     ERI    MIN II 11.26:.
BK     ERI    DS=8. P VAR.
BL     ERI    EMEHT HATC B POBEPKE./THE ELEMENTS
              SHOULD BE CHECKED.
BM     ERI    P>20000D; D=321D; D=270D.
              HAAETC TOKO OH MIN./ONLY ONE MIN WAS OB-
              SERVED.
              BHE MIN, COACHO/OUTSIDE MIN, ACCORDING TO  5828!,
              DV=0.2M, MAX=2440643.0+30D*E.
BQ     ERI    MIN II 10.9.
BV     ERI    MIN II 8.42. DII=0.06P.
BW     ERI    MIN II 9.72.
BY     ERI    (K-D)2=0.06.
BZ     ERI    MIN II 9.21.
CC     ERI    SB. MU=0.310", P=169G, PI=0.083". OTOMETPECK P
              OK K PORB./PHOTOMETRIC P IS CLOSE TO PORB.
              PEHTEHOBCK CTOHK./X-RAY SOURCE.
CI     ERI    VB (9.9M, 11.2M, 2", 106G).
CO     ERI    MIN II 9.1.
CS     ERI    (K-D)2=0.03.
CT     ERI    MIN II 10.27.
CW     ERI    MIN II 8.86, DII=0.10P.
DL     ERI    PO-CM.TA./SEE TABLE; P1=0.118795D  9206!; P2=
              =0.0968D  9207!.
DM     ERI    ADS 3380 (5.1M, 5.4M, 0.3", 161G). A BHA KAK
              BOHA  B 1877  1923./DUPLICITY WAS OBSER-
              VED ONLY IN 1877 AND 1923.
DO     ERI    AHA OXA MIN.OC C P-6.14 MH; BB-
              EHO 7 PAHX ACTOT. EH, PB=12.25D+-0.47D.
              MAX AMT OC OT COBAAET C MAX
              MAHTHOO O, AMTA MEHETC C PROT. CM-
              MAPHA AMTA OC 0.062M B./EPOCH OF
              MIN IS GIVEN. OSCILLATIONS WITH P-6.14 MIN, 7 DIFFE-
              RENT FREQUENCIES HAVE BEEN FOUND. BEAT PHENOMENON,
              PB=12.25D+-0.47D. MAX OF THE OSCILLATION AMPLITUDE
              ALMOST COINCIDES WITH MAX OF THE MAGNETIC FIELD, THE
              AMPLITUDE VARIES WITH PROT. COMBINED AMPLITUDE OF OS-
              CILLATIONS 0.062M B.
DS     ERI    MIN II 10.3. P VAR. MIN=2423147.25+0.827737D*E
              (J.D.2414869-23150); B HTEPBAE/DURING J.D.
              2423150-31320-CM.TA./SEE TABLE.
DW     ERI    ADS 3409 B (A 6.72M, G8III; B 9", 317G).
DY     ERI    ADS 3093 C (A 4.43M V, K1V; B 9.51M V, DA, 82",
              105G; BC A=7", PORB=252.1YR). MU=4.05", P=212G.
              PEHTEHOBCK CTOHK./X-RAY SOURCE.
DZ     ERI    AHA OXA/EPOCH IS GIVEN FOR MAX (Y), MIN (HE I).
              P=3.67D BOMOEH/IS POSSIBLE.
EF     ERI    2A0311-227. VB A (B 15.8M, 18", 260G). MU ALFA=+0.147",
              MUDELTA=-0.070". AHA OXA KOO MIN B K AX.
              COHA KAPTHA ATMEH OCAHA B  4041!. OC-
               C P-20.2  13.7 MH  9211!. KTA-
               ECKA./EPOCH OF NARROW MIN IN IR LIGHT IS GI-
              VEN. THE COMPLEX PHENOMENON OF ECLIPSES IS DESCRI-
              BED IN  4041!. OSCILLATIONS WITH P-20.2 AND 13.7 MIN.
               9211!. FLICKERING.
EG     ERI    AHA OXA MIN B AX Y./EPOCH OF MIN IN Y
              LIGHT IS GIVEN.
EH     ERI    ADS 3305 A (B 10.8M, 1.45", 60G, 1917).
GAMMA  ERI    ADS 2904 A (B 12.4M, 53", 242G).
LAMBDA ERI    B CEKTPE BPEMEHAM PHAK OOOK./SHELL
              FEATURES ARE SOMETIMES PRESENT IN THE SPECTRUM.
NU     ERI    SB? P2=0.1735079D. EH./BEAT EFFECT.
OMIKRO 1 ERI  P0-CM.TA./SEE TABLE. P1=0.1291D.
R*4    ERI    ADS 2472 A (B 9.9M, 6", 288G; C 11M, 40", 99G).
R*9    ERI    SB 1 (PORB=5.954D). P=1.2135D HE CKEH/IS NOT
              EXCLUDED.
S      FOR    VB (9.2M, 9.3M, 0.28", 358G, 1964).
              TPEM OTHM HAATEM B EBPOE B OH
              HO HAAAC HEOHO PKO, HA CHMKAX AP-
              BAPCKO OCEPBATOP B T E HO A B HOPMA-
              HOM ECKE./FOUND UNUSUALLY BRIGHT ONLY ON ONE NIGHT
              BY THREE EXPERIENCED OBSERVERS IN EUROPE; HARVARD PHO-
              TOGRAPHS OF THE SAME NIGHT SHOW IT IN NORMAL BRIGHTNESS.
V      FOR    (B-V)MAX=+0.26.
W      FOR    MIN II HAAETC/IS OBSERVED.
RX     FOR    (K-B)2=0.06.
RY     FOR    (B-V)MAX=+0.535.
SS     FOR    (K-B)2=0.09.
SW     FOR    DS>10:.
SY     FOR    SB 2  M+PEC(EQ)!.
TZ     FOR    SB 2. BOMOHE HAEH P:/POSSIBLE P VALUES:
              37.805D; 44.18D; 50.46D; 75.61D. D I=1D.
R      GEM    VB A (B 11.4M PG, 173", 200G, 1910). S 3.5/6E-S 6.5/6-.
S      GEM    VB A (B 11.1M, 70", 122G).
T      GEM    S 3/4E.
U      GEM    MIN=2437638.82685+0.17690602D*E+5.4D*10**-12*E**2
               9215!. HA MIN/DEPTH OF MIN 0.5M-1.0M.
              OCAHE CEKTPA/SPECTRUM DESCRIPTION  9216!.
V      GEM    P VAR. MAX=2407750+276.2D*E (J.D.2407700-15500);
              MAX=2415729+278.3D*E (J.D.2415600-21600); MAX=
              =2421839+269.8D*E (J.D.2421700-26500)  0458!; MAX=
              =2432580+281.3D*E (J.D.2427500-32600); MAX=
              =2434739+269.8D*E (J.D.2432600-35800); OCE/
              SINCE J.D.2435800 - CM.TA./SEE TABLE.
W      GEM    P VAR. MAX=2429815.990+7.914553D*E (J.D.2413200-
              31700); OCE/SINCE J.D.2431700 - CM.TA./SEE
              TABLE.  A/H!=0.2.
              BOMOHO HAE CAOO OOO CTHKA/
              THERE IS POSSIBLY FAINT BLUE COMPANION.
RR     GEM    P VAR. MAX=2415219.734+0.39729235D*E (J.D.
              2412000-18000); MAX=2418278.900+0.39727274D*E
              (J.D.2418000-21000); MAX=2422865.229+
              +0.39724027D*E (J.D.2421000-25000)  9217!; MAX=
              =2427150.267+0.3972596D*E (J.D.2426200-27850);
              MAX=2434806.289+0.3973103D*E (J.D.2428200-
              34900)  2392!; OCE/SINCE J.D.2436000 - CM.TA./
              SEE TABLE.
              EKT AKO/BLAZHKO EFFECT, PB=48D  3618!,
              PB=37D  9221!. DS=3.
RW     GEM    VB A (B 11.04M, 20", 105G; C 11.84M, 100", 120G).
              MIN II 9.74; D=0.02P.
RX     GEM    VB A (B 12.65M, 45", 215G). MIN II 9.28; D=0.004P.
              P VAR. MIN I=2417970.0+12.20868D*E (J.D.2415000-
              27500)  7534!; OCE/SINCE J.D.2427600 - CM.TA./
              SEE TABLE.
              EMEHT, PBEEHHE B TAE, COEPAT KBA-
              PATH EH:/THERE IS A SQUARE TERM IN THE ELE-
              MENTS GIVEN IN THE TABLE:+2.25D*10**-7*E**2.
              ABH KOMOHEHT CCTEM OKPEH CBETM-
              C AOBM KOOM/LUMINOUS GASEOUS RING SUR-
              ROUNDS THE PRIMARY COMPONENT OF THE SYSTEM  7535!.
RY     GEM    VB A (B 12.30M, 45", 240G). MIN II 8.75; D=0.023P.
              P VAR. MIN I=2418015.333+9.300876D*E (J.D.
              2418000-33000)  8653!; OCE/SINCE J.D.2433000-
              CM.TA./SEE TABLE.
              KOMOHEHT KACCA A OKPEH CBETMC AOBM
              KOOM./COMPONENT OF A TYPE IS SURROUNDED BY A
              LUMINOUS GASEOUS RING.
RZ     GEM    VB. P VAR. MAX=2429632.453+5.529716D*E (J.D.
              2415000-32400); OCE/SINCE J.D.2432400 - CM.
              TA./SEE TABLE.
SS     GEM    9.9M=<MIN II=<10.7M.
SU     GEM    P VAR. MIN I=2429204+50.12D*E (J.D.2429200-355)
               0310!; MIN I=2437772.5+50.39D*E (J.D.2437739-
              39850); MIN I=2439856.6+50.10D*E (J.D.2439850-
              40680); OCE/SINCE J.D.2440680 - CM.TA./SEE
              TABLE.
              EMEHT MEHEH CPEHEO ECKA:/MEAN BRIGHT-
              NESS VARIES WITH THE ELEMENTS: MIN=2437953+680D*E;
              M-M=264D.
              AMTA KOPOTKOEPOECKX MEHEH/AMP-
              LITUDE OF SHORTPERIODICAL VARIATIONS IS 0.3M-0.9M.
SW     GEM    AHA OXA MIN ECKA./MIN BRIGHTNESS EPOCH IS
              GIVEN.
SX     GEM    MIN II 11.3; D=0.05P:.
TX     GEM    HA MIN II/DEPTH OF MIN II 0.04M; D=0.017P:.
UV     GEM    VB A (B 19.5M, 7", 285G).
WW     GEM    MIN II 10.3.
WY     GEM    MOET T ATMEHHO CCTEMO, OOHO VV CEP.
              B 1960-61 . HAAOC ATMOCEPHOE ATMEHE,
              CEPEHA KOTOPOO PXOTC HA 1968 .  5730!.
              EPEMEHHOE MAHTHOE OE  1591, 4498!. BOMO-
              HA TAKE ECKA EPEMEHHOCT OOO KOM-
              OHEHTA  7536!./MAY BE AN ECLIPSING SYSTEM SIMI-
              LAR TO VV CEP. ATMOSPHERIC ECLIPSE BEGAN PROBABLY
              IN 1960-61, THE MEAN PHASE OF IT BEING IN 1968
               5730!. VARIABLE MAGNETIC FIELD  1591, 4498!. INTRIN-
              SIC VARIABILITY OF BLUE COMPONENT IS ALSO POSSIBLE
               7536!.
YY     GEM    VB C (A 1.99M, B 2.85M, A=6.06", P=306.3 Y; C 73",
              165G, 1925); MU ALFA=-0.0154S,MU DELTA=-0.108". MIN II    ;
9.59
              MIN II-MIN I=0.50P; D=0.000P. X-CTOHK/X-RAY
              SOURCE. P SONST  8655!.
              OA KOMOHEHTA, O-BMOM, BTC EPEMEH-
              HM TA UV CET. AMTA BCEK B HTE-
              PAHOM ECKE CCTEM OCTAET 0.3MV, 
              1.8MU/BOTH COMPONENTS ARE PROBABLY UV CET TYPE
              VARIABLES. FLARE AMPLITUDE IN THE INTEGRATED LIGHT OF
              THE SYSTEM REACHES 0.3MV, OR 1.8MU  9227!.
AA     GEM     A/H!=0.0.
AC     GEM    MIN II 11.3. P VAR. MIN I=2433649.30+1.661795D*E
              (J.D.2415000-36000)  1530!; OCE/SINCE J.D.
              2430100 - CM.TA./SEE TABLE.
AF     GEM    VB A (B 14.8M, 2", 0G). MIN II 10.67. EMEHT, AH-
              HE B TAE, COEPAT KBAPATH EH:/THERE
              IS A SQUARE TERM IN THE ELEMENTS GIVEN IN THE TABLE:
              -1.71D*10**-10*E**2.
AH     GEM    MIN II 14.8:.
AI     GEM    MIN II 14.0.
AL     GEM    MIN II 9.85.
AN     GEM    MIN II 13.3:; D=0.037P.
AU     GEM    OH MCC/EMISSION.
AV     GEM    MIN II 12.8:.
AY     GEM    MIN II 10.9.
AZ     GEM    MIN II 12.4.
BB     GEM    VB A (B 12M, 25", 270G).
BP     GEM    P VAR. MAX=2434120+243.9D*E (J.D.2418700-36600);
              OCE/SINCE J.D.2436600 - CM.TA./SEE TABLE.
BT     GEM    MIN II 14.0:.
CI     GEM    UG?
CM     GEM    MIN II 15.0.
DL     GEM    VB A (B 13.1M, 18", 180G).
DN     GEM    VB A (B 13.5M, 12", 16G; C 12.0M, 80", 99G).
DP     GEM    MIN II 14.0. RRC? P=0.2792D?
DX     GEM    P VAR. MAX=2433182.876+3.136226D*E (J.D.2425000-
              34000); MAX=2435554.199+3.136955D*E (J.D.
              2434000-36500)  8300!; OCE/SINCE J.D.2436500-
              CM.TA./SEE TABLE.
EF     GEM    P VAR. MIN=2428108.49+6.10222D*E (J.D.2428500-
              42800)  0407!; OCE/SINCE J.D.2442800 - CM.TA./
              SEE TABLE.
EL     GEM    MIN II 13.6.
EN     GEM    MIN II 13.8.
EW     GEM    P VAR. MAX=2428495.686+0.523750D*E (J.D.2428100-
              30780); OCE/SINCE J.D.2430780 - CM.TA./SEE
              TABLE.
EY     GEM    MIN II 13.0.
FT     GEM    MIN II 14.1.
GP     GEM    MIN II 13.5.
GR     GEM    15.6=<MIN II=<15.9.
GW     GEM    MIN II 10.68.
GX     GEM    MIN II 11.3.
GZ     GEM    P=1.225290D?
HH     GEM    MIN II 13.8.
HR     GEM    MIN II 11.7.
HY     GEM    MIN II 17.5.
II     GEM    P=223D?
IP     GEM    MIN II 14.5.
IR     GEM    B CBEPXMAKCMMAX - KOEAH C P=102 MH./IN SUPER-
              MAXIMA THERE ARE SUPERHUMPS WITH P=102 MIN  9232!.
IZ     GEM    D>=0.24D.
KQ     GEM    MIN II 14.6.
KU     GEM    D=0.05P.
KV     GEM    AHA OXA MIN ECKA. O CEKTP BOMOEH T
              EW  9037!./EPOCH OF MIN OF BRIGHTNESS IS GIVEN. EW
              TYPE IS POSSIBLE ACCORDING TO THE SPECTRUM  9037!.
KZ     GEM    BOMOHO, K PABEH 129D/THE CYCLE MAY BE 129D.
LM     GEM    D=0.02P.
LX     GEM    KPACHA./RED.
MO     GEM    KPACHA./RED.
MP     GEM    VB.
MU     GEM    MIN II 14.9.
MZ     GEM    MIN II 16.7.
NQ     GEM    B EBPAE 1970 . B EPOHOM CEKTPE OBC
              MCCOHHE H BOOPOA  TPAOETOBA
              HEPEPBHA MCC/IN THE SPECTRUM OF THE CARBON
              STAR THE HYDROGEN EMISSION LINES AND ULTRAVIOLET CON-
              TINUOUS EMISSION APPEARED IN FEBRUARY 1970  6348!.
NY     GEM    HD 47396 (PEC)=S 5438=K 798=K 6468. HA
              KAPTE B  0156! OOEHE EPEMEHHO KAAHO HE-
              BEPHO./IN THE CHART IN  0156! THE POSITION OF THE VA-
              RIABLE IS WRONG.
OS     GEM    HA KOEAH C EPOOM P1, PBEEHHM B TA-
              E, HAKABATC KOEAH C EPOOM P0=
              =0.070D C MEHE AMTO./OSCILLATIONS WITH
              THE PERIOD P1 GIVEN IN THE TABLE ARE SUPERIMPOSED
              BY OSCILLATIONS WITH THE PERIOD P0=0.070D AND SMAL-
              LER AMPLITUDE. P1/P0=0.78.
       GEM    VB A (B 11.46M, 87", 84G; C 7.56M, 97", 350G). P VAR.
              MAX=2410640.42+10.15477D*E (J.D.2394600-
              2407150); MAX=2422366.187+10.15288D*E (J.D.
              2407150-22300); MAX=2426802.918+10.15172D*E
              (J.D.2422300-34500)  2392!; OCE/SINCE J.D.
              2434500 - CM.TA./SEE TABLE.
              BCE HAEH PECTABTC TAKE EMEHTA-
              M:/ALL THE OBSERVATIONS ARE SATISFIED ALSO BY THE
              ELEMENTS: MAX=2443785.444+10.150135D*E-
              5.24D*10**-7*E**2  9029!.
              BOMOHO, OTHOCTC K T DCEPS./MAY BY A
              DCEPS TYPE VARIABLE.
ETA    GEM    VB A (B 8.8M, GO III-IV, 1.60", 269.4G, 1977). SB 1
              (P=2983D  9236!). AHA OXA MIN ECKA. HAO-
              EE OKE MIN, COOTBETCTBE CEPEHAM HC-
              XOX BETBE KPBO VR, OBETBOPTC E-
              MEHTAM:/EPOCH OF MIN BRIGHTNESS IS GIVEN. THE
              DEEPEST MINIMA (CORRESPONDING TO THE MIDDLES OF THE
              DESCENDING BRANCHES OF THE RADIAL VELOCITY CURVE) ARE
              SATISFIED BY THE ELEMENTS: MIN=2429355+2984D*E
               1551!.
MU     GEM    VB A (B 9.8M, 122", 141G).
SIGMA  GEM    VB A (B 10.8M, 182", 316G); SB 1 (P=19.603D  9238!).
              HA KPBO ECKA HAAETC MIN II, HOA C-
              EA, HOA CTAHOBC E MIN I./
              THERE IS A MIN II ON THE LIGHT CURVE; MIN II SOMETIMES
              DISAPPEARS AND SOMETIMES BECOMES DEEPER THEN MIN I.
              MIN II-MIN I=0.5P.
U      GRU    HA/DEPTH OF MIN II 0.05M. D=0.011P.
W      GRU    P VAR. KBAPATH EH:/NONLINEAR TERM:+7.84D*
              *10**-9*E**2. MIN II 10.0.
X      GRU    D=0.008P. MIN II 10.69. P VAR. AH TEKE E-
              MEHT./CURRENT ELEMENTS ARE GIVEN.
Z      GRU    DS=12:. OPMA KPBO ECKA  P CHO MEHT-
              C./THE SHAPE OF THE LIGHT CURVE AND P ARE STRONGLY
              VARIABLE.
RS     GRU    (K-B)2=0.22.
RT     GRU    (K-B)2=0.02. EKT AKO./BLAZHKO EFFECT.
RV     GRU    (B-V)MAX=+0.93. MIN II 11.4.
RW     GRU    DS=10. EKT AKO./BLAZHKO EFFECT.
RX     GRU    MIN II 10.7.
RY     GRU    HAOEHE HEPABHX KOEAH?/SUPERPOSITION
              OF IRREGULAR VARIATIONS?
              B HTEPBAE/DURING J.D.2434513-517 PEBC-
              EHHE MHMM HE HAAC./PRECALCULATED
              MINIMA WERE NOT OBSERVED.
RZ     GRU    OCAHE MEHEH ECKA  2809!./A DESCRIPTION
              OF LIGHT CHANGES  2809!.
UW     GRU     FE/H!=-1.6.
VW     GRU    P>=260D?
VY     GRU    P>160D.
VZ     GRU    BOMOEH TAKE T RR./RR TYPE IS ALSO POSSIBLE.
AK     GRU    EMEHT HATC B OTBEPEH./ELEMENTS
              SHOULD BE CHECKED.
AP     GRU    P VAR. CPEHE EMEHT/MEAN ELEMENTS J.D.
              2427992-36848 - CM.TA./SEE TABLE. B HTEPBAE/
              DURING J.D.2434250-36848 MAX=2434337.337+
              +0.5082945D*E.
AR     GRU    MIN II 10.6.
AV     GRU    P>=160D BOMOEH./IS POSSIBLE.
AW     GRU    MIN II? J.D.2436818.
BC     GRU    MIN II 10.3. BOMOEH T RRC./RRC TYPE IS POS-
              SIBLE.
BD     GRU    MIN II 14.9.
BH     GRU    MIN II 15.2:.
PI1    GRU    VB A (B 10.9M, GOV, 2.7", 202G).
T      HER    VB A (B 10M, 67", 321G).
U      HER    SIO, OH, H2O MAEP/MASER.
W      HER    ADS 10121 A (B 14.2M, 6", 334G).
X      HER    P2=746D.
Z      HER    VB A (B RO>10"). MIN II 8.18. KBAPATH EH:/
              NONLINEAR TERM:-6.19D*10**-10*E**2.
RU     HER    SIO MAEP/MASER. B MIN ECKA CEKTP KOMHPO-
              BAHH; CTHK?  33502!./THE SPECTRUM IN MIN
              LIGHT IS COMPOSITE; A COMPANION?  3502!.
RX     HER    MIN II 7.74.
SW     HER    B-V; +0.12, +0.40. P VAR. O/BEFORE 1921 MAX=
              =2416687.018+0.4928864D*E.
SX     HER     FE/H!=-1.8.
SY     HER    O MEHEHX EPOA CM.  8699!./ON PERIOD VARIA-
              TIONS SEE  8699!.
SZ     HER    MIN II 10.10. P VAR. MIN=2430766.8390+0.818096D*E+
              +0.0165D SIN (0.010465G*E+180G)  5749!. B TAE-
              TEKE EMEHT, OBETBOPTEHE OCE J.D.
              2438000./THE TABLE GIVES CURRENT ELEMENTS SATISFAC-
              TORY AFTER J.D.2438000.
TT     HER    MIN II 9.89. OPMA KPBO ECKA/THE LIGHT CURVE
              SHAPE VAR.
              P VAR. O/BEFORE J.D.2430000 MIN=2425433.627+
              +0.9120846D  2389!; MIN=2434525.2572+0.9120800D*E
              (J.D.2430000-40000)  3504!;  OCE/SINCE J.D.
              2440000 - CM.TA./SEE TABLE.
TU     HER    D=0.022P. P VAR. O/BEFORE J.D.2435000 MIN=
              =2424381.416+2.2671303D*E-854D*10**-11*E**2  9240!;
              MIN=2437462.3909+2.2669718D*E (J.D.2435000-
              38000)  9241!; MIN=2443324.70097+2.2669385D*E
              (J.D.2438000-44000)  8593!; OCE/SINCE  J.D.
              2444000 - CM.TA./SEE TABLE.
TW     HER     FE/H!=-0.47.
TX     HER    MIN II 8.97, DII=0.11P. P VAR; EPOECK EH:/
              PERIODIC TERM:+0.0081D SIN  0.042G (E+7255)!.
UU     HER     FE/H!=-1.27. HAAOC EPEOBAHE EPOOB
              90D  71D  0310!; OTMEAC TAKE EPO 45D
               3507!./ THERE WAS ALTERNATION OF PERIODS 90D AND 71D
               0310!; THE PERIOD 45D  3507! WAS ALSO NOTED.
              B HTEPBAE/DURING J.D.2443611-44161 - CM.TA./
              SEE TABLE.
              AHA OXA MIN./EPOCH OF MIN IS GIVEN.
UX     HER    MIN II 9.11. P VAR. O/BEFORE J.D.2429000 MIN=
              =2419876.467+1.5488598D*E  0279!; MIN=
              =2429987.420+1.5488513D*E (J.D.2429000-38000)
               3671!; OCE/SINCE J.D.2438000 - CM.TA./SEE
              TABLE.
VW     HER    VB A (B 17.3M, 18", 120G).
VX     HER    DS=5. P VAR; KBAPATH EH:/NONLINEAR TERM:
              -0.00745D (E:10000)**2.
              COACHO  3369!,  MOET T EHOM ATMEHHO-
              BOHO CCTEM./ACCORDING TO  3369!, POSSIBLY IS
              A MEMBER OF AN ECLIPSING BINARY SYSTEM.
VZ     HER     FE/H!=-0.9. P VAR. P=0.44031880D (J.D.2415000-
              22000)  5738!; MAX=2425004.4590+0.44032394D*E
              (J.D.2422000-27000); MAX=2425004.4456+
              +0.44032631D*E (J.D.2427000-36000)  3506!; OCE/
              SINCE J.D.2436000 - CM.TA./SEE TABLE.
WW     HER    VB A (B 15.6M, 7.4", 148.5G, E/WHITE).
WX     HER    HE CKEH BBOE O P./TWICE LONGER P IS
              NOT EXCLUDED.
AC     HER    P VAR. B TAE - TEKE EMEHT, ECTBE
              OCE J.D.2442000. B CPEHEM P=75.4619D  1754!.
              BEHA B MAX KOEETC C DM=1.6M  0368!./THE
              TABLE GIVES CURRENT ELEMENTS VALID SINCE J.D.
              2442000. MEAN P=75.4619D  1754!. THE MAGNITUDE IN
              MAX VARIES WITH DM=1.6M  0368!.
AD     HER    VB A (B 11.97M, 5", 189G). D=0.033P. MIN II 9.79.
AF     HER    P VAR. O/BEFORE J.D.2426950 P=0.630336D; OCE/
              SINCE J.D.2426950 - CM.TA./SEE TABLE.
              OPMA KPBO ECKA/THE SHAPE OF THE LIGHT CURVE
              VAR.
AG     HER    P VAR. MAX=2422935.584+0.6494378D*E (J.D.
              2418210-26952); OCE/SINCE J.D.2426952 - CM.TA./
              SEE TABLE.
AH     HER    PORB=5.9D:. CA BO BPEM BCEK:/OSCILLA-
              TIONS DURING OUTBURSTS: 24S=<P=<39S, DM=<0.003M  9251!.
              KOEAH B MAX  MIN O 0.4M A BPEM OT 2 O
              8 MH/FLICCKERING IN MAX AND MIN UP TO 0.4M IN 2-
              8 MINUTES  9252!.
AK     HER    ADS 10408 A (B 12.0M, 5", 323G). MIN II 8.64. MIN II-
              -MIN I=0.505P. DII=0.07P. P VAR. O/BEFORE J.D.
              2421200 MIN=2421200.549+0.42152207D*E; MIN=
              =2421200.549+0.42152083D*E (J.D.2421200-24950);
              MIN=2424949.555+0.42152061D*E  (J.D.2424950-
              30000)  1760!; MIN=2430939.368+0.42152362D*E
              (J.D.2430000-41500); OCE/SINCE 2441500 - CM.
              TA./SEE TABLE.
              OPMA KPBO ECKA/THE SHAPE OF THE LIGHT CURVE
              VAR.
AM     HER    U 1809+50. LX(SOFT)/LOPT-15.
              B CEKTPE MCC H  KCAII, H, HEI, HEII  P.
              AHA OXA MIN I B AX V. EPO MEHETC CO-
              HM OPAOM. AA MIN I B AX U 0.30P, B AX B
              0.15P, B AX R 0.05P. MIN I, BEPOTHO, OCOBEH
              ATMEHEM OPEO THA  CTP  OBEPXHOC-
              T EOO KAPKA CAMM EM KAPKOM. -
              HA MIN I O 0.7M. MIN II HO O 0.4M (HOA
              OTCTCTBET), MIN II-MIN I=0.55P. MIN II COBAAET
              O AE C PEHTEHOBCKM ATMEHEM. AKTBHE 
              HEAKTBHE CTA (B-13.0M  B-15.0M B CPEHEM);
              B AKTBHO CTA KOEAH C DM-0.3M C XAPAK-
              TEPHM BPEMEHEM>=200D; POOTEHOCT HE-
              AKTBHX CTA 130D-700D  9258!  MEHEE. BO
              BPEM HEAKTBHX COCTOH HA MHMMOB
              MAA. KTA ECKA O 0.8MV A HECKOKO
              MHT  ECTKOB CEKH; KTA B PEHTE-
              HOBCKOM AAOHE A BPEM -10S, HE KOPPEP-
              E C OTECKM. MAHTHOE OE - 1*10**7 C HA
              KBATOPE, -2*10**7 C HA OCAX. EPEMEHHA KP-
              OBA (OT +3% O -9%)  HEHA (O 7%) OP-
              A. K TOK HA LAMBDA 10 MKM./EMISSIONS OF H AND
              KCAII, H, HEI, HEII, ETC. IN THE SPECTRUM. EPOCH OF
              MIN I IN V LIGHT IS GIVEN. THE PERIOD SHOWS COMPLEX
              VARIATIONS. THE PHASE OF MIN I IN U LIGHT IS 0.30P, IN
              B 0.15P, IN R 0.05P. MIN I IS PROBABLY DUE TO AN EC-
              LIPSE OF A HOT SPOT AND THE GAS FLOW NEAR THE SURFACE
              OF THE WHITE DWARF BY THE WHITE DWARF ITSELF. THE
              DEPTH OF MIN I IS UP TO 0.7M. MIN II WITH THE DEPTH UP
              TO 0.4M (SOMETIMES ABSENT), MIN II-MIN I=0.55P. MIN II
              COINCIDES  IN PHASE WITH THE X-RAY ECLIPSE. HIGH AND
              LOW STATES (B-13.0M AND B-15.0M ON AVERAGE); IN
              THE HIGH STATE THERE ARE VARIATIONS WITH DM-0.3M ON
              THE TIME SCALE>=200D; THE DURATION OF LOW STATES IS
              130D-700D  9258! OR LESS. DURING LOW STATES THE
              DEPTH OF MINIMA IS SMALL. FLICKERING UP TO 0.8MV IN
              SEVERAL MINUTES OR DOZENS OF SECONDS; X-RAY FLICKE-
              RING ON THE TIME SCALE OF -10S NOT CORRELATING WITH
              OPTICAL FLICKERING. THE MAGNETIC FIELD - 1*10**7 G AT
              THE EQUATOR, -2*10**7 G ON POLES. VARIABLE CIRCULAR
              (FROM +3% TO -9%) AND LINEAR (UP TO 7%) POLARIZATION.
              IR EXCESS AT LAMBDA 10 MUM.
AP     HER    P VAR CHO/STRONGLY. P=10.400D (J.D.2415000-
              19000:); P=10.3970D (J.D.2423700-24700:); P=
              =10.4260D (J.D.2424700-25300); P=10.4338D (J.D.
              2425800-27000); P=10.3945D (J.D.2427000-27400);
              P=10.4277D (J.D.2433000-33850); P=10.3898D (J.D.
              2433850-34850);=P=10.4209D (J.D.2434850-35600);
              P=10.3715D (J.D.2435600-37200); B HTEPBAE/
              DURING J.D.2437200-43800 - CM.TA./SEE TABLE.
              OPMA KPBO ECKA/THE LIGHT CURVE SHAPE VAR.
               A/H!=-0.8.
AR     HER    P VAR COHM OPAOM/IN A COMPLICATED WAY. MAX=
              =2424794.274+0.4700234D*E (1905-1954)  6535!;
              MAX=2439692.683+0.469975D*E (1954-1967)  5274!;
              OCE/SINCE 1967 - CM.TA./SEE TABLE.
              EKT AKO/BLAZHKO EFFECT, =31.5489D  3555!,
              DM VAR (0.9M-:1.8MPG)  2168!, (M-M) VAR. DS=6.
AT     HER    PKA HA OHO ACTHKE/THE STAR IS BRIGHT ON ONE
              PLATE (J.D.2418209).
              B OCTAHOE BPEM/BESIDES THAT, 11.8M-12.25M.
AW     HER    VB A (B 10"-20"). D=0.03P.
BB     HER    P VAR. P=7.507696D (J.D.2418924-30700); OCE/
              SINCE J.D.2430700 - CM.TA./SEE TABLE.  A/H!=
              =+0.3.
BC     HER    P VAR. O/BEFORE J.D.2432000 MIN=2426242.372+
              +3.08752D*E  9262!; OCE/SINCE J.D.2436000 - CM.
              TA./SEE TABLE.
BD     HER    P VAR. P=0.4739135D (J.D.2426540-29620); P=
              =0.4739057D (J.D.2429620-30570); MAX=2430495.404+
              +0.4739126D*E (J.D.2430570-O/BEFORE 1948)  9263!;
              OCE/SINCE 1948 - CM.TA./SEE TABLE. DS=0.8.
BL     HER    P VAR. P=1.3074604D (J.D.2415000-35000); OCE/
              SINCE J.D.2435000 - CM.TA./SEE TABLE.
              PO BAPAHT PECTABEH:/ANOTHER POSSIBLE
              REPRESENTATION: MAX=2434999.402+1.307457D*E
              -3.9D*10**-10*E**2 (J.D.2415000-42000).  FE/H!=0.0.
BO     HER    D=0.015P. MIN II 10.8. P VAR?
CC     HER    P VAR. MIN=2426120.415+1.7340314D*E (J.D.
              2425790-31265); MIN=2431265.288+1.7340460D*E
              (J.D.2431265-36000)  2389!; MIN=2439668.342+
              +1.73398D*E (J.D.2436000-39600); OCE/SINCE J.D.
              2439600 - CM.TA./SEE TABLE.
CD     HER    KAPTA B  6286! HEBEPHA./THE CHART IN  6286! IS
              WRONG.
CE     HER     A/H!=-1.8.
CK     HER    P VAR? MAX=2429231.234+0.519201D*E (J.D.2429231-
              877)  0332!; B HTEPBAE/DURING J.D.2436041-
              37955 - CM.TA./SEE TABLE.
CO     HER    P2=600D. HOA HE MEHETC B TEEHE 150D./SO-
              METIMES DOES NOT VARY FOR 150D.
CP     HER    HAKABATC BOH/SUPERIMPOSED WAVES, 50D-
              100D.
CT     HER    HA MIN II/THE DERTH OF MIN II 0.05M. P VAR.
              MIN=2430904.431+1.786337D*E (J.D.2426480-35000)
               3567!; MIN=2439355.666+1.7863645D*E (J.D.
              2435000-39500)  0001!; MIN=J.D.2441499.3307+
              +1.7863891D*E (J.D.2439500-42500)  8593!; OCE/
              SINCE J.D.2442500 - CM.TA./SEE TABLE.
DE     HER    P VAR. MAX=2425754+171.2D*E (J.D.2425754-30890);
              MAX=2430889+175.3D*E (J.D.2430890-36150); B H-
              TEPBAE/DURING J.D.2436150-38140 - CM.TA./SEE
              TABLE.
DF     HER    EMEHT CPABEB OCE/ELEMENTS ARE VALID
              SINCE J.D.2425900.
DH     HER    D=0.024P:. MIN II 9.5.
DI     HER    MIN II 8.95, DII=0.03P, MIN II-MIN I=0.77P (1966-
              1978). BPAEHE H AC:/APSIDAL MOTION: P=
              =29000YR+-4000YR;MIN II=2442241.4602+
              +10.5501751D*E.
              HATEHOE POTBOPEE ME HAAEMO 
              TEOPETECKO  CKOPOCT BPAEH H AC./
              A CONSIDERABLE DISCREPANCY BETWEEN THE OBSERVED AND
              THE THEORETICAL RATE OF APSIDAL MOTION.
DK     HER    P VAR.
DL     HER    EKT AKO/BLAZHKO EFFECT, =33.6D, 11.0M=<
              =<MMAX=<11.3M. P VAR. DS=5.
DO     HER    POM C/CLOSE TO V362 HER.
DQ     HER    VB A (B 18.17M, F, 3.5", 132G, OTECK?/OPTICAL?).
              TMAHHOCT/NEBULA, R=10.5" (HALFA, 1981). OCE
              ABHOO MAX HOBO HAAC OK MIN 13.0M
              (J.D.2426925)  OCK BTOPH MAX 6.7M (J.D.
              2427065)./AFTER THE MAIN MAX OF THE NOVA A DEEP
              MIN 13.0M (J.D.2426925) AND A FLAT SECONDARY MAX
              6.7M (J.D.2427065) WERE OBSERVED.
              ATMEHHA EPEMEHHOCT:/ECLIPSING VARIABILITY:
              14.61M-18.08M, MIN HEI=2434954.9445+0.193620877D*E
               9280!. D=0.20P, D=0.000P.
              OPMA KPBO ECKA  DM/THE LIGHT CURVE SHAPE
              AND DM VAR.
              CA:/OSCILLATIONS: MAX HEI=JED
              2434954.785868+8.22521640D*10**-4*E-2.8048D*10**-16*E**2
               8722!, 0=<DM=<0.08M.
              MEHEH OPA C BOEHHM EPOOM OC-
              ./POLARIZATION CHANGES WITH DOUBLE OSCIL-
              LATION PERIOD.
              KTA:/FLICKERING: DM=0.15M.
DY     HER    P VAR, KBAPATH EH:/NONLINEAR TERM:-18.6D*
              *10**-13*E**2.
EI     HER    KPACHA./RED.
EN     HER    P VAR. O/BEFORE J.D.2427000 P=160D.
ES     HER    MIN II 13.7.
ET     HER    EMEHT OBETBOPT HAEHM O/THE ELE-
              MENTS ARE VALID EARLIER THAN J.D.2427200
EX     HER    KPACHA./RED.
EZ     HER    EMEHT OBETBOPT HAEHM O/THE ELE-
              MENTS ARE VALID EARLIER THAN J.D.2427400.
FN     HER    P VAR?
FW     HER    MIN II 14.6.
FY     HER    O CEKTP BOMOEH T EW./ACCORDING TO THE
              SPECTRUM, EW TYPE IS POSSIBLE.
GL     HER    P VAR?
GU     HER    D=0.010P. MIN II 11.8. MIN II-MIN I=0.513P.
GV     HER     FE/H!=-1.41. P VAR. MAX=2427543.360+
              +0.2914606D*E (J.D.2427543-29728)  0152!; B HTEP-
              BAE/DURING J.D.2436041-38170 - CM.TA./SEE
              TABLE.
GY     HER    P VAR. MAX=2428219.623+0.524347D*E (J.D.2428219-
              727)  0152!; B HTEPBAE/DURING J.D.2436370-
              38170 - CM.TA./SEE TABLE.
HS     HER    D=0.025P. MIN II 8.63. P VAR; OCE/SINCE J.D.
              2438240 - CM.TA./SEE TABLE.
              BPAEHE H AC:/APSIDAL MOTION: -130YR
               6538!.
HV     HER    D=0.008P:; MIN II 12.9:.
HZ     HER    HER X-1=4U 1656+35. LX/LOPT=2-60. B TAE-
              EMEHT  MHMMOB ECKA, CBAHHX C AT-
              MEHHO EPEMEHHOCT  EKTOM OTPAEH.
              MIN I ECKA COBAAT C PEHTEHOBCKM ATME-
              HM. BOMOEH HEOO MIN II. EKTOM OT-
              PAEH OCOBEHA EPEMEHHOCT C DM O 1.5M.
              B PEHTEHOBCKX AX HAAETC K 34.875D;
              CTOHK CA B TEEHE 2/3 KA. HAAETC
              EPEMEHHOCT OPM OTECKO KPBO ECKA B
              TEEHE 35-HEBHOO KA  9283!. COACHO  6539!,
              B HTEPBAAX J.D.2427543-657  J.D.2428630-
              29789 CH EKT OTPAEH OTCTCTBOBA;
              BEA POOAA MEHTC C P=1.7D  MEA
              DM-0.5M, MIN I=MIN II. O AHHM  6546!, TAKE
              HTEPBA OTCTCTB EKTA OTPAEH POO-
              TEHOCT OT 8D O 7A C 1890 . AHMA
              OT OOBH BPEMEH. BO BPEM TAKX COCTO-
              H HAATC MEHEH ECKA B PEEAX
              14.7M-15.2M PG. C 1957 . COCTOH E EKTA
              OTPAEH HE HAAOC. B HE-E 1983 .
              OAEME COCTOH BCOKOO PEHTEHOBCKOO
              ECKA HE HACT, OHAKO PEKPAEH EKTA
              OTPAEH HE POOO  9284!. BTOPHE KOE-
              AH ECKA: P1=1.0977D (DB1=0.33M), P2=
              =0.871173D*E (DB2=0.10M), P3=1.623846D*E (DB3=
              =0.17M)  9285!. PEHTEHOBCK CAP, P=
              =1.2377991S (J.D.2443357), P/P=(-2.9+-0.2)*
              *10**-6/O  9286!, HOA POBC B OTE-
              CKOM AAOHE  6543!. CTPE KTA EC-
              KA./THE TABLE GIVES ELEMENTS FOR LIGHT MINIMA DUE
              TO ECLIPSING VARIABILITY AND THE REFLECTION EFFECT. MIN I
              COINCIDES WITH THE X-RAY ECLIPSE. SHALLOW MIN II MAY
              BE PRESENT. THE REFLECTION EFFECT CAUSES VARIATIONS
              WITH DM UP TO 1.5M. A CYCLE OF 34.875D DURATION IS
              OBSERVED IN X-RAY BAND; THE SOURCE IS FAINT DURING
              TWO THIRDS OF THE CYCLE. THE OPTICAL LIGHT CURVE CHAN-
              GES ARE OBSERVED DURING THE 35D CYCLE  9283!. AC-
              CORDING TO  6539!, DURING J.D.2427543-657 AND J.D.
              2428630-29789 THE STRONG REFLECTION EFFECT WAS AB-
              SENT; THE STAR WAS STILL VARYING WITH P=1.7D AND HAD
              DM-0.5M, MIN I=MIN II. IN  6546! IT IS STATED THAT
              SUCH INTERVALS WITH NO REFLECTION EFFECT, OF 8D TO 7A
              DURATION, TOOK PLACE FOR ALMOST HALF THE TIME SINCE
              1890. THE LIGHT CHANGES DURING SUCH INTERVALS ARE IN
              THE RANGE 14.7M-15.2M PG. SINCE 1957 INTERVALS WIT-
              HOUT THE REFLECTION EFFECT WERE NOT OBSERVED. IN JUNE-
              JULY 1983 THE PREDICTED PHASES OF HIGH X-RAY FLUX
              DID NOT TAKE PLACE, BUT THE REFLECTION EFFECT DID NOT
              DISAPPEAR  9284!. SECONDARY LIGHT VARIATIONS: P1=
              =1.0977D (DB1=0.33M), P2=0.871173D*E (DB2=0.10M),
              P3=1.623846D*E (DB3=0.17M)  9285!. X-RAY PULSAR,
              P=1.2377991S (J.D.2443357), P/P=(-2.9+-0.2)*
              *10**-6/YR  9286!, SOMETIMES NOTICEABLE ALSO IN THE
              OPTICAL RANGE  6543!. RAPID BRIGHTNESS FLICKERING.
IK     HER    D=0.030P?
IQ     HER    HAOEHE KOEAH C OEE KOPOTKM P  MAO
              DM/SUPERPOSITION OF VARIATIONS WITH SHORTER P AND
              SMALL DM  6645!.
IT     HER    CM./SEE FY HER.
KL     HER    MIN II 14.7.
KV     HER    KPBA ECKA XAPAKTEPHA  BE TA MP K-
              TA, HO CHO MEHETC. MHOO HEPABHOCTE./
              THE LIGHT CURVE IS CHARACTERISTIC OF MIRA CETI STARS
              BUT STRONGLY VARIES. MANY IRREGULARITIES. O-C: -96D,
              +73D.
LR     HER    MIN II 15.4:.
LS     HER    OPMA KPBO ECKA VAR./THE LIGHT CURVE SHAPE VAR.
LT     HER    D=0.02P. MIN II 10.79.
LV     HER    P VAR? B HTEPBAE/DURING J.D.2428429-31342 - CM.
              TA./SEE TABLE.
MM     HER    VB A (B 13.50M, 18", 120G). MIN II 9.7. DM BOH HA
              KPBO ECKA O/DM OF THE DISTORSION WAVE UP TO
              0.12M.
MP     HER     FE/H!=-1.18.
MS     HER    MIN II 13.3.
MT     HER    MIN II 12.30.
MV     HER    HA KAPTE B  0156! EPEMEHHA OTMEEHA HEBEPHO;
              HA CAMOM EE EPEMEHHO MV HER BETC BE-
              A, OTMEEHHA KAK "C"./THE CHART IN  0156! IDEN-
              TIFIES THE VARIABLE ERRONEOUSLY; REAL MV HER IS MAR-
              KED AS "C".
MW     HER    P VAR. P=503D (1976)  9290!. B HTEPBAE/DURING
              J.D.24668-29172 - CM.TA./SEE TABLE.
MX     HER    MOMEHT MIN OCE J.D.2444000, OKOBAHHE
              PAHM PAM HAATEE, HAXOTC B
              POTBOPE ME COO./MOMENTS OF MIN AFTER
              J.D.2444000 PUBLISHED BY DIFFERENT GROUPS OF OBSER-
              VERS CONTRADICT EACH OTHER.
NQ     HER    COACHO/ACCORDING TO  3882!, EA, 8.0-8.6 PG, MIN II
              8.4, MIN I=2426894.433+0.870218D*E (J.D.2426894-
              34250).
NR     HER    BOH/WAVES, P=2.8D-5.5D.
OQ     HER    AHA OXA MIN./EPOCH OF MIN IS GIVEN.
OS     HER    B-V:+0.12, +0.48.
OU     HER    CEKTPAH KACC AH COACHO  2198!./SPECTRAL
              TYPE IS GIVEN ACCORDING TO  2198!; B/IN BSD-G7.
OX     HER    DS=6:.
PW     HER    MIN II 10.1; DII-0.3P( ).
V338   HER    MIN II 10.13. P VAR. O/BEFORE J.D.2437000 MIN=
              2433771.38+1.305732D*E  3115!; MIN=2441864.379+
              +1.3057515D*E (J.D.2437000-43400)  8593, 0001!; O-
              CE/SINCE J.D.2443400 - CM.TA./SEE TABLE.
V342   HER    MIN II 10.7.
V347   HER    P VAR. MAX=2415288.21+0.5373619D*E (J.D.2415288-
              18596); OCE/SINCE J.D.2429495 - CM.TA./SEE
              TABLE.
V359   HER    P VAR. MIN=2416046.476+1.755754D*E (J.D.2416000-
              26500)  0001!; MIN=2435693.47+1.755775D*E (J.D.
              2426500-36000)  1040!; OCE/SINCE J.D.2443500-
              CM.TA./SEE TABLE.
V362   HER    POM C/CLOSE TO DO HER.
V365   HER    EKT AKO:/BLAZHKO EFFECT: =40.64D. P VAR.
              B HTEPBAE/DURING J.D.2429037-36840 - CM.TA./
              SEE TABLE.
V373   HER    P=0.33D /OR 0.50D BOMOEH/IS POSSIBLE.
V384   HER    CM./SEE V373 HER.
V387   HER    MIN II 13.2.
V394   HER    P VAR?
V395   HER    Z=0.0643.
V396   HER    Z=0.175.
V403   HER    MIN II 16.0:.
V412   HER    MIN II 15.2.
V422   HER    P VAR? B HTEPBAE/DURING J.D.2434131-35991-
              CM.TA./SEE TABLE.
V423   HER    MIN II 15.0.
V426   HER    MIN II 15.8.
V431   HER    P VAR.
V436   HER    EMEHT HEBEPEHHE./THE ELEMENTS ARE UNCER-
              TAIN.
V441   HER    K TOK, PHAK OKOOBEHO OOOK.
              BOMOH HEPAAHE CA./IR EXCESS,
              EVIDENCE FOR A CIRCUMSTELLAR ENVELOPE. POSSIBLY NON-
              RADIAL PULSATION.
V442   HER    P VAR. MAX=2434223.375+0.4421143D*E (J.D.
              2417447-36083); OCE/SINCE J.D.2435730 - CM.
              TA./SEE TABLE.
              OPMA KPBO ECKA MEHETC./THE SHAPE OF THE
              LIGHT CURVE VARIES.
V446   HER    O BCK/BEFORE THE OUTBURST 16.2M-18.8M  3607!.
V451   HER    ADS 10310 A (B 10.70M, 19", 239G). AHA OXA MIN
              B AX U./ THE EPOCH OF MIN U LIGHT IS GIVEN.
V458   HER     FE/H!=-1.65.
V463   HER    P=54.4D BOMOEH/IS POSSIBLE.
V477   HER    MIN II 15.4.
V482   HER    BOMOHO, ATMEHHA/POSSIBLY ECLIPSING.
V499   HER    EKT AKO./BLAZHKO EFFECT.
V502   HER    MIN II 13.5?
V510   HER    P VAR?
V511   HER    P VAR?
V513   HER    MIN II 15.7.
V516   HER    MIN II 17.1.
V523   HER    EMEHT ECTBT B HTEPBAE/ELEMENTS ARE VA-
              LID DURING J.D.2430940-990.
V524   HER    BOMOEH BBOE MEH P./TWICE SHORTER P IS
              POSSIBLE.
V527   HER    MAX=2430938.451+0.5188D*E (J.D.2430938-990); B
              HTEPBAE/DURING J.D.2436308-318 - CM.TA./SEE
              TABLE.
V529   HER    AHA OXA MIN./EPOCH OF MIN IS GIVEN.
              COACHO/ACCORDING TO  4217!, P=120D.
V533   HER    VB A (B 16M, 9.5", 0G). CA:/OSCILLATIONS:
              MAX=2443717.730281+0.0007364941D*E, A-1%
               4162!.
V551   HER    P=4.00D/N BOMOEH/IS POSSIBLE.
V552   HER    P=3.04D/N BOMOEH/IS POSSIBLE.
V554   HER    P=4.01D/N BOMOEH/IS POSSIBLE.
V557   HER    P=8.00D/N BOMOEH/IS POSSIBLE.
V570   HER    P=0.5D /OR 0.33D BOMOEH/IS POSSIBLE.
V578   HER    KPACHA./RED.
V582   HER    VB. KPACHA./RED.
V583   HER    KPACHA./RED.
V588   HER    BOMOHO, ATMEHHA./POSSIBLY ECLIPSING.
V600   HER    SB, PORB- CM.TA./SEE TABLE.
              EPEMEHHOCT VR, BOMOHO, CBAHHA C CA-
              M TA BCEP:/VARIABILITY OF VR POSSIBLY CAU-
              SED BY BCEP TYPE PULSATIONS: P-0.18D.
V601   HER    EMEHT PECTABT HAEH OCE/ELE-
              MENTS ARE VALID SINCE J.D.2439184.
V604   HER    KPACHA./RED.
V608   HER    EKT AKO./BLAZHKO EFFECT.
V615   HER    KPACHA./RED.
V618   HER    P VAR?
V624   HER    VB A (12.04M, 40"). MIN II 6.35. SB 2.
V637   HER    ADS 10227 A (BC 9.2M, 9.2M, 1.7", 18G, 1975; BC: A=
              =0.28", PORB=56.56YR).
V639   HER    MU ALFA=-0.21", MU DELTA=+0.39",PI=0.087". VB B (A=V647   ,
HER
              11.36M VAR, DM4E; B 16", 268G). BCK B AX U
               PG./FLARES IN THE BANDS U AND M PG.
V640   HER    VB A (B 14.9M, 8.5", 217G; C 13.9M, 23", 221G).
V641   HER    BOMOEH TAKE T L  ISB./L OR ISB TYPE IS
              ALSO POSSIBLE.
V644   HER    SB (PORB=11.859D).
V645   HER    P-3H-10H, K/A CYCLE OF 40D.
V647   HER    VB A (B=V639 HER, 16", 268G); MU ALFA=-0.21", MU DELTA=
              =+0.39"; PI=0.087".
V652   HER    P VAR; KBAPATH EH: NONLINEAR TERM:-45.80D*
              *10**-10*E**2. DM VAR.
              CXOHA CO BEAM TA PV TEL, HO BETC
              EEBM CKAPKOM. AHA OXA MAX. BTOP-
              H OP HA AE 0.5P./RESEMBLES PV TEL TYPE
              STARS BUT IS A HELIUM RICH SUBDWARF. EPOCH OF MAX IS
              GIVEN. SECONDARY HUMP AT THE PHASE 0.5P.
V654   HER    DM=0.15M B EOM CBETE/IN WHITE LIGHT.
V655   HER    ADS 10407 A (B 9.2M, 4.1", 144G, 1971).
V657   HER    COACHO/ACCORDING TO  2610!, CST?, 11.0M.
V662   HER    MEHEE BEPOTHE HAEH P:/LESS PROBABLE P VA-
              LUES: 0.56629D, 0.56710D, 0.56881D, 0.56970D.
V685   HER    MIN II 15.8.
V687   HER    MIN II 14.9.
V691   HER    BOMOHE HAEH P:/POSSIBLE P VALUES: 0.927D,
              0.637D.
V697   HER    H2O, OH MAEP/MASER.
V699   HER    MIN II 16.0:.
V717   HER    EKT AKO?/BLAZHKO EFFECT?
V718   HER    MIN II 14.3.
V719   HER    HE CKEH T EW C BOEHHM HAEHEM P./
              EW TYPE WITH TWICE LONGER P IS NOT EXCLUDED.
V720_  V721   HER CM./SEE V717 HER.
V722   HER    MIN II 15.7.
V723   HER    MIN II 15.5.
V728   HER    MIN II 11.4.
V731   HER    MIN II 13.8. HE CKEHO OOBHHOE HAEHE P./
              TWICE SHORTER P IS NOT EXCLUDED.
V732   HER    MIN II 13.8.
V733   HER    MIN II 14.3:.
V737   HER    CM./SEE V717 HER.
V740   HER    MIN II 14.4.
V741   HER    CM./SEE V717 HER.
V742   HER    MIN II 14.4.
V744   HER    VR VAR, P=86.7221D (SB1? HEPAAHE CA?/
              NONRADIAL PULSATION?).
              BOMOHA CTPA CEKTPAHA EPEMEHHOCT:/
              RAPID SPECTRAL VARIABILITY IS POSSIBLE: P=2.5552D,
              0.78906D.
V749   HER    P=465S.
V771   HER    AHA OXA MAX B AX U./EPOCH OF MAX U LIGHT
              IS GIVEN.
V772   HER    VB AB (7.4M, GOV; 8.5M, G8V:; A=0.27", E=0.97, P=
              =20.0YR, C 10.62M, 28"). OH  KOMOHEHTOB
              (O-BMOM, B)-SB1, P=0.879511D  4056!. OH E
              OEBHO, BETC ATMEHHO CCTEMO. CA
              PEHTEHOBCK CTOHK./ONE OF THE COMPONENTS
              (PROBABLY B) IS SB1, P=0.879511D  4056!. THE SAME
              COMPONENT MUST BE THE ECLIPSING SYSTEM. FAINT X-RAY
              SOURCE.
V774   HER    HAP CO BCKAM HAATC "AHTBCK"
              CPABHMO AMT - PEKE OCAEH ECKA./
              BOTH FLARES AND "ANTIFLARES" (ABRUPT FADINGS) OF COM-
              PARABLE AMPLITUDE ARE OBSERVED.
ALFA   HER    ADS 10418 A (B 5.39M, 4.9", 107G, 1973; B-SB2, G5III+
              +F2V). MEEHHE KOEAH, P-6 ET, DM-0.5M;
              OEE CTPE, P-50D-155D, DM-0.3M-1.0M. BMEC-
              TE C BAHM CTHKOM OKPEHA OPOMHO OO-
              OKO (R-2*10**5R$, CKOPOCT PACPEH 10 KM/C,
              OTEP MACC 3*10**-8M$/O)./SLOW VARIATIONS, P-
              -6YR, DM-0.5M; QUICKER CHANGES, P-50D-155D, DM-
              -0.3M-1.0M. TOGETHER WITH THE VISUAL COMPANION THE
              STAR IS SURROUNDED BY AN ENORMOUS ENVELOPE (R-2*10**5R$,
              EXPANSION VELOCITY 10 KM/S, MASS LOSS 3*10**-8M$/YR).
NU     HER     FE/H!=-0.26. SB?
OMIKRO HER    VB HTEPEPOMETPECKA./INTERFEROMETRIC.
OMEGA  HER    ADS 10054 A (B 11.5M, 0.8", 232G, 1967; C 11.0M, 28.4",
              96G, 1957; D 27.5", 271G, 1960). AHA OXA MIN. HA
              KPBO ECKA BOHA BOHA. CTPE MEHEH,
              P=0.15D  9310!./EPOCH OF MIN IS GIVEN. DOUBLE WAVE
              IN THE LIGHT CURVE. RAPID VARIATIONS, P=0.15D  9310!.
G      HER    AH CPEH K 1972-1981. HAKABATC ME-
              EHHE CA (<P>=875D+-70D)  HEEPOEC-
              KE KOEAH C XAPAKTEPHM BPEMEHEM 5D-15D 
              DM O 0.2M./THE MEAN CYCLE 1972-1981 IS GIVEN. SLOW
              PULSATIONS (<P>=875D+-70D) AND NON-PERIODIC VARIA-
              TIONS ON THE TIME SCALE OF 5D-15D WITH DM UP TO
              0.2M ARE SUPERIMPOSED.
U      HER    ADS 10449 A (B 10.2M, 4.4", 60G). MIN II 4.93.
R      HOR    OH, H2O, SIO MAEP/MASER. P VAR. MAX=2428868+
              +401.5D*E (J.D.2412800-28900); OCE/SINCE J.D.
              2428900 - CM.TA./SEE TABLE.
V      HOR    <P>=59D (J.D.2428380-910), <P>=90D (J.D.
              2429170-980).
X      HOR    AHA OXA MIN ECKA. MAKCMM POKE. O-
              HO HAATC BTOPHE MHMM./EPOCH OF
              MIN BRIGHTNESS IS GIVEN. MAXIMA ARE BROAD. USUALLY
              SECONDARY MINIMA ARE OBSERVED.
SY     HOR    MIN II 12.0.
SZ     HOR    MIN II 10.7:.
TU     HOR    MIN II 6.03; MIN II-MIN I=0.52P; MAX II HA 0.05M CA-
              EE, EM MAX I. EKPHA COAHA E-
              PEMEHHA/MAX II IS FAINTER THAN MAX I BY 0.05M. PE-
              CULIAR ELLIPSOIDAL VARIABLE  9245!.
TY     HOR    T/TYPE RCB?
UU     HOR    P VAR. MAX=2416826.417+0.6436900D*E (J.D.
              2416800-25000); OCE/SINCE J.D.2425000 - CM.
              TA./SEE TABLE.
UX     HOR    MIN II 14.4. P VAR. MIN I=2426659.380+0.7126943D*E
              (J.D.2426650-30860); OCE/SINCE J.D.2430540-
              CM.TA./SEE TABLE.
UZ     HOR    P VAR. MAX=2426679.425+0.338188D*E (J.D.2426300-
              28430); OCE/SINCE J.D.2430040 - CM.TA./SEE
              TABLE.
VY     HOR    MU=0.173", RO=33G. P=314S, 617S.
R      HYA    VB A (B 13.0M, 21.6", 324G). SIO MAEP/MASER.
              P VAR. COACHO/ACCORDING TO  0458!; MAX=
              =2328201+486D*E (J.D.2328200-31120); MAX=
              =2343512+507D*E (J.D.2343300-44800); MAX=
              =2372678+485D*E (J.D.2372200-72700); MAX=
              =2380447+477D*E (J.D.2380000-81400); MAX=
              =2385160+461D*E (J.D.2384700-88000); MAX=
              =2394350+448.6D*E (J.D.2393900-2402000); MAX=
              =2403742+434D*E (J.D.2403300-04200); MAX=
              =2406363+429.5D*E (J.D.2406000-11100); MAX=
              =2413642+411D*E (J.D.2413200-14100); MAX=
              =2416563+405.5D*E (J.D.2416100-23400); MAX=
              =2424288+414.7D*E (J.D.2423400-28500). OCE/
              SINCE J.D.2428500 - CM.TA./SEE TABLE.
T      HYA    P VAR. MAX=2399455+289.00D*E(J.D.2398600-
              2421700); MAX=2422584+294.2D*E (J.D.2421700-
              25800); MAX=2431781+284.20D*E (J.D.2425800-
              36200); OCE/SINCE J.D.2437500 - CM.TA./SEE
              TABLE.
V      HYA    VB A (B 11.58MV, KO III, 46", 186G). KOEAH EC-
              KA C AMTO OT 1.1M, O 2M  EMEHTAM, P-
              BEEHHM B TAE, HAKABATC HA MEHEH
              CPEHEO ECKA C P=6670D  AMTO 3.5M.
              OKE MHMM ECKA HAAC B 1891,
              1908, 1925, 1942-43, 1959  1962 . PAK CBO-
              HO KPBO ECKA  3614!./MEAN BRIGHTNESS VARIA-
              TIONS WITH P=6670D AND A=3.5M ARE SUPERIMPOSED
              BY LIGHT OSCILLATIONS WITH A=1.1M-2M AND ELEMENTS
              GIVEN IN THE TABLE. DEEP LIGHT MINIMA WERE OBSER-
              VED IN 1891, 1908, 1925, 1942-43, 1959,  AND 1962.
              A GRAPH OF THE LIGHT CURVE  3614!.
W      HYA    VB A (B 9.3M, 72", 108G). P VAR. MAX=2411074+
              +379D*E (J.D.2411000-14150); MAX=2414644+
              +395D*E (J.D.2414150-19400); MAX=2419746+
              +378D*E (J.D.2419400-25200)  0458!. MAX=
              =2425740+366D*E (J.D.2425200-27000); MAX=
              =2440336+397.35D*E (J.D.2428000-40500); OCE/
              SINCE J.D.2440500 - CM.TA./SEE TABLE.
              AMTA  OPMA KPBO ECKA CHO MEHT-
              C./AMPLITUDE AND SHAPE OF THE LIGHT CURVE VARY
              STRONGLY.
              OH, H2O, SIO MAEP/MASER.
X      HYA    OH, H2O, SIO MAEP/MASER.
Y      HYA    CPEH BEHA MEHETC./MEAN MAGNITUDE VA-
              RIES.
RR     HYA    H2O MAEP/MASER.
RS     HYA    P VAR. MAX=2422973+330.2D*E (J.D.2414000-23000);
              MAX=2429126+342.0D*E (J.D.2423000-29200); MAX=
              =2429455+331.2D*E (J.D.2429200-34500); OCE/
              SINCE J.D.2434500 - CM.TA./SEE TABLE.
RT     HYA    O/BEFORE 1952 <P>=255D; OCE/SINCE 1952 - CM.
              TA./SEE TABLE.
              XAPAKTEP  AMTA MEHEH ECKA CHO ME-
              HTC./THE CHARACTER AND AMPLITUDE OF LIGHT VARIA-
              TIONS VARY STRONGLY.
RU     HYA    OH, H2O MAEP/MASER. P VAR. MAX=2429572+
              +334.0D*E (J.D.2414000-29600); OCE/SINCE J.D.
              2428500 - CM.TA./SEE TABLE.
RW     HYA    SB 2 (P=370D). AHA OXA MIN ECKA./EPOCH
              OF MIN BRIGHTNESS IS GIVEN.
RX     HYA    VB A (B 10.5M). HA/DEPTH OF MIN II 0.05M. P VAR.
              MIN I=2428261.385+2.2815942D*E (J.D.2419500-
              28500); MIN I=2440650.409+2.2816200D*E (J.D.
              2428500-41400); OCE/SINCE J.D.2441400 - CM.
              TA./SEE TABLE.
SS     HYA    VB A (B 12.0M, 13", 195G); SB 2.
SU     HYA    CPEH BEHA MEHETC C P=780D./MEAN MAG-
              NITUDE VARIES WITH P=780D.
SV     HYA    VB A (B 35", 225G). DS=7.
SX     HYA    D=0.022P. P VAR. MIN I=2427659.223+2.895697D*E
              (J.D.2410000-28000)  0007!; OCE/SINCE J.D.
              2442500 - CM.TA./SEE TABLE.
SY     HYA    P VAR. MIN=2425590.589+3.403082D*E (J.D.2425500-
              31150)  7548!. OCE/SINCE J.D.2432200 - CM.TA./
              SEE TABLE.
SZ     HYA    P VAR. MAX=2415714.1429+0.53742815D*E (J.D.
              2414700-26500)  3626!; MAX=2426410.575+0.53736D*E
              (J.D.2426400-27200)  0001!; MAX=2431881.5537+
              +0.53723051D*E (J.D.2427880-35200)  3626!; MAX=
              =2435542.267+0.5372497D*E (J.D.2435500-38900)
               3627!. OCE/SINCE J.D.2438770 - CM.TA./SEE
              TABLE.
              EKT AKO/BLAZHKO EFFECT: MAX(A)=2440705+
              +25.8D*N  6557!; 10.44M=<MAX=<11.03M.
TT     HYA    MIN II 7.32; D=0.035P.
TU     HYA    P VAR. MAX=2416980+277.5D*E (J.D.2412500-
              17300); MAX=2417260+272.5D*E (J.D.2417200-
              19800)  1787!; MAX=2430410+281.4D*E (J.D.
              2420500-30500); MAX=2438332+272.3D*E (J.D.
              2432000-39200); OCE/SINCE J.D.2439200 - CM.
              TA./SEE TABLE.
TY     HYA    P VAR. MIN=2434478.464+4.660978D*E (J.D.2419800-
              35000)  1788!; OCE/SINCE J.D.2435000 - CM.TA./
              SEE TABLE.
UU     HYA    P VAR. MAX=2427423.84+0.5238585D*E (J.D.2414950-
              27400)  1789!; MAX=2429729.835+0.523854D*E (J.D.
              2427000-31000)  0752!. CEKTP-O CA II/SPECTRUM
              IS BASED ON CA II.
UW     HYA    MIN II 13.8:; MIN II-MIN I=0.64P. P=1.055439D?
UY     HYA    MIN II 13.8. RRC?
VV     HYA    P VAR. MAX=2427421+155D*E (J.D.2419500-37000)
               1792!; OCE/SINCE J.D.2437000 - CM.TA./SEE
              TABLE.
VX     HYA    (K-B)2=0.26. KACC CBETMOCT  3149! POTBOPE-
              T T EPEMEHHOCT ECKA. OPMA KPBO EC-
              KA CHO MEHETC. HA OCHOBHOE KOEAHE C E-
              POOM P0, AHHM B TAE, HAKABAETC BTO-
              PHOE C P1=0.172720D  3631!./LUMINOSITY CLASS
               3149! CONTRADICTS THE TYPE OF LIGHT VARIABILITY. THE
              SHAPE OF THE LIGHT CURVE STRONGLY VARIES. THE MAIN
              OSCILLATION WITH THE PERIOD P0 GIVEN IN THE TABLE IS
              SUPERIMPOSED BY THE SECONDARY ONE WITH P1=0.172720D
               3631!. P1/P0=0.773; PB=0.761445D.
VY     HYA    MIN II 9.1.
VZ     HYA    MIN II 9.46.
WY     HYA    MIN II 11.2.
WZ     HYA    (K-B)2=0.06. P VAR. MAX=2416169.681+0.53772640D*E
              (J.D.2414000-19000); MAX=2419811.736+
              +0.53775858D*E (J.D.2419000-21000); MAX=
              =2424618.630+0.53774101D*E (J.D.2421000-32000)
               0752!; MAX=2436613.445+0.5377229D*E (J.D.
              2436600-38500)  3633!; OCE/SINCE J.D.2438000-
              CM.TA./SEE TABLE.
XX     HYA    P VAR. MAX=2439560.355+0.50774868D*E (J.D.
              2428200-39560)  5238!; OCE/SINCE J.D.2439560-
              CM.TA./SEE TABLE.
XZ     HYA    MIN II 15.0.
AE     HYA    MIN II 14.6.
AF     HYA    MIN II 13.8.
AI     HYA    MIN II 9.84; MIN II-MIN I=0.438P; DII=0.075P; DI=0.02P;
              DII=0.00P; EA/DM. EPO CA P'/PULSATION
              PERIOD P'=0.13803D, A=0.02M-0.03M  9259!.
AV     HYA    MIN II 10.35; DI=0.023P:.
CH     HYA    MIN II 15.5; MIN II-MIN I=0.57P.
CW     HYA    P VAR?  4027!. PBEEHHE B TAE EMEHT
              OBETBOPT HAEHM TOKO B HTEPBAE
              J.D.2428950-30375./ELEMENTS GIVEN IN THE TABLE
              SATISFY OBSERVATIONS ONLY IN THE INTERVAL J.D.
              2428950-30375.
DD     HYA    P VAR. MAX=2431139.313+0.501818D*E (J.D.2431100-
              600)  1432!. OCE/SINCE J.D.2441600 - CM.TA./
              SEE TABLE.
DE     HYA    D=0.014P?
DF     HYA    MIN II 11.5.
DH     HYA    DS=7.
DK     HYA    MIN II 10.7.
DM     HYA    D=0.15P?
EU     HYA    MIN II 10.2.
EX     HYA    MEHEH ECKA C PORB  AMTO O 0.9MV,
              O'CHEC ATMEHEM OPEO THA, PE-
              CTABTC EMEHTAM: ET(MIN)=2437699.94177+
              +0.0682338422D*E, E ET(MIN)-EOEHTPEC-
              KA AHCKA ATA, PEBPAEHHA B EMEPHOE
              BPEM; OHOBPEMEHHO HAAETC EPOECKA
              MO OPM KPBO ECKA ME BCKA-
              M C AMTO OT 0.2M O 0.9M  EMEHTAM:
              MAX=2437699.8895+0.04654656D*E-1.2D*10**-12*E**2
               9265!. CPEH HTEPBA ME PKM BCKA-
              M 465D  5695!, CPEH K-HA OPOK MEHE./
              LIGHT VARIATIONS WITH PORB AND AMPLITUDE UP TO 0.9MV
              DUE TO ECLIPSES OF HOT SPOT ARE REPRESENTED BY THE
              ELEMENTS: ET(MIN)=2437699.94177+0.0682338422D*E,
              WHERE ET(MIN) IS THE HELIOCENTRIC JULIAN DATE CON-
              VERTED TO EPHEMERIS TIME; SIMULTANEOUSLY PERIODIC
              MODULATION OF THE SHAPE OF THE LIGHT CURVE BETWEEN
              THE OUTBURSTS IS OBSERVED WITH THE AMPLITUDE 0.2M-
              0.9M AND THE ELEMENTS: MAX=2437699.8895+
              +0.04654656D*E-1.2D*10**-12*E**2  9265!. MEAN INTER-
              VAL BETWEEN BRIGHT OUTBURSTS IS 465D  5695!, MEAN
              CYCLE IS CLOSE TO 20-30D.
EY     HYA    P VAR. MAX=2432707+160.5D*E (J.D.2426100-32800);
              OCE/SINCE J.D.2432800 - CM.TA./SEE TABLE.
EZ     HYA    MIN II 10.7. P VAR. MIN I=2440255.8482+
              +0.44976658D*E (J.D.2431160-40650)  7549!; OCE/
              SINCE J.D.2440250 - CM.TA./SEE TABLE.
FG     HYA    MIN II 10.25; DI=DII=0.085P. P VAR. MIN I=
              =2431150.388+0.3278422D*E (J.D.2431140-34400)
               0182!; MIN I=2436968.7067+0.32783433D*E (J.D.
              2434050-400)  3639!; MIN I=2436968.7067+
              +0.32783546D*E (J.D.2436950-43250)  9267!; OCE/
              SINCE J.D.2444600 - CM.TA./SEE TABLE.
FI     HYA    V27 B APOBOM CKOEH NGC 4590 (M68); HE EH
              CKOEH./V27 IN THE GLOBULAR CLUSTER NGC 4590
              (M68); CLUSTER NON-MEMBER.
FS     HYA    COACHO/ACCORDING TO  1480! P=91.7D.
FW     HYA    MIN II 12.4.
FY     HYA    VB A (B 15.45M, 15", 90G); DS=7:; (K-B)2=-0.03.
GK     HYA    MIN II 9.57. EMEHT COEPAT KBAPATH
              EH:/THERE IS A SQUARE TERM IN THE ELEMENTS:
              -4.01D*10**-9*E**2.
GM     HYA    D=<0.01P.
GN     HYA    MIN II 13.6.
GT     HYA    CEP?
HS     HYA    MIN II 8.55.
IK     HYA    EKT AKO C =30D/BLAZHKO EFFECT WITH =
              =30D.
IW     HYA    OH, H2O MAEP/MASER.
KM     HYA    P VAR?
KU     HYA    VB AB (7.3M, 7.4M, A=0.150", P=58.93 YR, E=0.219);
              A(V)=0.06M.
KW     HYA    PORB=7.75043D; E=0.110  9273!; MIN II 6.35; MIN II-
              -MIN I=0.54P.
BETA   HYA    VB A (B 5.6M, 0.9", 8G, 1959).
HI     HYA    MIN II 5.92.
R      HYI    EH MAOO MAEAHOBA OAKA./THE MEMBER OF
              THE SMALL MAGELLANIC CLOUD.
Y      HYI    D=0.024P.
RS     HYI    B PAOHE MAOO MAEAHOBA OAKA. HE EH O-
              AKA./IN THE REGION OF THE SMALL MAGELLANIC CLOUD.
              NOT A MEMBER OF THE CLOUD.
RT     HYI    MIN II 14.1.
RV     HYI    MIN II 12.4; MIN II-MIN I=0.61P.
RY     HYI    CM./SEE RS HYI.
RZ     HYI    CM./SEE R HYI.
ST     HYI    CM./SEE R HYI.  A/H!=-0.8.
SZ     HYI    CM./SEE RS HYI.
TW     HYI    DS=10:.
UU     HYI    P=112.25D?
VW     HYI    CPEH HTEPBA ME CBEPXMAKCMMAM 179D.
              PORB=0.0742711D. ME HOPMAHM BCKAM
              ECK EPOECK BOPACTAET HA 0.35M-0.40M, B
              CB C  OBEHM OPEO THA: MAX=
              =2440128.0222+0.0742711D*E  7550!. BO BPEM
              CBEPXMAKCMMOB EPO ME OOHM "OPA-
              M" PABEH 0.0769D  9275!. HOA HAATC
              KTA ECKA C AMTO 2%  KOM OT
              28 O 34 CEKH  7551!./MEAN INTERVAL BETWEEN THE
              SUPERMAXIMA IS 179D. PORB=0.0742711D. BETWEEN THE
              NORMAL OUTBURSTS THE BRIGHTNESS PERIODICALLY INCREA-
              SES BY 0.35M-0.40M BECAUSE OF HOT SPOT APPEARANCES:
              MAX=2440128.0222+0.0742711D*E  7550!. DURING THE
              SUPERMAXIMA THE PERIOD BETWEEN THE SUPERHUMPS IS
              0.0769D  9275!. SOMETIMES THE LIGHT OSCILLATIONS WITH
              THE AMPLITUDE 2% AND CYCLE FROM 28S TO 34S ARE OB-
              SERVED  7551!.
VY     HYI    CM./SEE RS HYI.
VZ     HYI    RR  0193!.
WX     HYI    CPEH HTEPBA ME CBEPXMAKCMMAM 141.5D.
              PORB=0.0748134D  9277!. EPO ME OPAM,
              HAAEMM BO BPEM CBEPXMAKCMMOB, PABEH
              0.07737D  9278!./MEAN INTERVAL BETWEEN THE SUPER-
              MAXIMA IS 141.5D. PORB=0.0748134D  9277!. PERIOD
              BETWEEN THE SUPERHUMPS OBSERVED DURING THE SUPER-
              MAXIMA IS 0.07737D  9278!.
WZ     HYI    CM./SEE RS HYI.
XY     HYI    CM./SEE R HYI.
AC     HYI    CM./SEE RS HYI.
AH     HYI    CM./SEE R HYI.
AI     HYI    CM./SEE R HYI.
BB     HYI    DS=7:.
V      IND    P VAR. MAX=2439792.276+0.4796030D*E (J.D.
              2414000-40000)  5233!; OCE/SINCE J.D.2440000-
              CM.TA./SEE TABLE.
              DS=7, (K-B)2=0.02.
RS     IND    MIN II 10.0. P VAR.
RU     IND    VB A (B 12.6M, 2.3", 103G). MIN II 12.1.
RX     IND    240D<P<310D.
RY     IND    MIN II 11.04.
ST     IND    MIN II 11.79.
SU     IND    MIN II 9.5:.
TV     IND    MIN II 11.9.
AR     IND    MIN II 14.4. RRC?
AY     IND    MU ALFA=+0.345", MU DELTA=-0.310"; VB?
R      LAC    VB A (B 14.1M, 6", 50G).
S      LAC    P VAR. MAX=2412857+238.2D*E (J.D.2410000-16400);
              MAX=2418828+241.45D*E (J.D.2416400-20500); MAX=
              =2427307+242.7D*E (J.D.2420500-27300); MAX=
              =2437290+237.4D*E (J.D.2427300-37300); OCE/
              SINCE J.D.2437300 - CM.TA./SEE TABLE.
U      LAC    HAATC  MEHEH ECKA C EPOAM:/THERE
              ARE LIGHT VARIATIONS WITH THE PERIODS: 150D, 550-690D,
              2900D.
V      LAC    P VAR. EMEHT COEPAT KBAPATH EH:/THERE
              IS A SQUARE TERM IN THE ELEMENTS: -6.48D*10**-8*E**2.
W      LAC    P VAR. MAX=2415255+323D*E (J.D.2414600-15300);
              MAX=2425628+335.5D*E (J.D.2425600-38000)  0458!;
              MAX=2433844+324.5D*E (J.D.2428000-33850); OCE/
              SINCE J.D.2433850 - CM.TA./SEE TABLE.
X      LAC    P VAR. MAX=2418890.497+5.444303D*E (J.D.2416670-
              29500)  2033!; OCE/SINCE J.D.2429500 - CM.TA./
              SEE TABLE.
Z      LAC    P VAR. EMEHT COEPAT KBAPATH EH:/
              THERE IS A SQUARE TERM IN THE ELEMENTS: -3.4D*10**-8*E**2.
               A/H!=0.2.
RR     LAC    P VAR. MAX=2419434.331+6.416146D*E (J.D.2417900-
              31600); OCE/SINCE J.D.2431600 - CM.TA./SEE
              TABLE.  A/H!=0.0.
RT     LAC    MIN II 9.62. P VAR. MIN I=2440382.9005+5.0740484D*E+
              +1.02D*10**-8*E**2 (J.D.2411650-42500)  8592!; OCE/
              SINCE J.D.2436470 - CM.TA./SEE TABLE.
              EMEHT, PBEEHHE B TAE, COEPAT KBA-
              PATH EH:/THERE IS A SQUARE TERM IN THE ELE-
              MENTS GIVEN IN THE TABLE: -2.7D*10**-8*E**2.
              OPMA KPBO ECKA  H MHMMOB MEH-
              TC. COACHO  9293! EPO MPA CTOPC-
              OHHO BOH - 9.5 ET, EPO MEHEH AMT-
               BOH (0<A=<0.17M) - 30 ET. COACHO  9292!,
              EPO MPA BBOE MEHE./SHAPE OF THE LIGHT
              CURVE AND DEPTHS OF THE MINIMA VARY. ACCORDING TO
               9293! THE PERIOD OF THE DISTORTION WAVE MIGRATION IS
              - 9.5 YR, THE PERIOD OF THE WAVE AMPLITUDE VARIATIONS
              (0<A=<0.17M) IS - 30 YR. ACCORDING TO  9292! THE
              MIGRATION PERIOD IS NEARLY HALF OF THE VALUE GIVEN IN
               9293!.
RV     LAC    CPEH BEHA MEHETC C EPOOM 550-700D./
              MEAN MAGNITUDE VARIES WITH THE PERIOD 550-700D.
RW     LAC    MIN II 10.8; DII=0.024P; MIN II-MIN I=0.492P.
RX     LAC    S7.5/1E. P=174D (J.D.2414950-29550)  1026!; OC-
              E/SINCE J.D.2436800 - CM.TA./SEE TABLE.
RY     LAC    HA KOEAH CPEHE BEH C P=300-420D 
              A=<0.5M HAKABATC KOEAH C P=38-91D./
              OSCILLATIONS OF MEAN MAGNITUDE WITH P=300-420D
              AND A=<0.5M ARE SUPERIMPOSED BY OSCILLATIONS WITH
              P=38-91D.
SS     LAC    BOMOH EH PACCEHHOO CKOEH/PROBABLE
              MEMBER OF THE OPEN CLUSTER NGC 7209. MIN II 10.5;
              MIN II-MIN I=0.57P; D=0.008P.
              BOMOHO BEHE H AC C P=1000 ET./
              APSIDAL MOTION WITH P=1000 YR IS POSSIBLE.
ST     LAC    EMEHT TPET POBEPK./ELEMENTS SHOULD BE
              CHECKED.
SU     LAC    P VAR. MAX=2412748+279.10D*E (J.D.2412700-
              27000)  5707!; MAX=2426972+286.74D*E (J.D.2426900-
              31000); MAX=2431008+306.0D*E (J.D.2431000-33150)
               0001!; MAX=2433150+319.14D*E (J.D.2433150-
              42150)  5707!; OCE/SINCE J.D.2442100 - CM.TA./
              SEE TABLE.
SW     LAC    MIN II 9.31. P VAR. MIN I=2418943.712+0.32071236D*E
              (J.D.2410000-19990); MIN I=2420038.621+
              +0.32071510D*E (J.D.2419990-25210); MIN I=
              2430996.525+0.32071665D*E (J.D.2425210-33690);
              MIN I=2436046.5634+0.32072132D*E (J.D.2433690-
              36755)  5222!; MIN I=2437572.5723+0.32072811D*E
              (J.D.2436755-40000)  3374!; MIN I=2440467.4592+
              +0.32072480D*E (J.D.2440110-40500)  6089!; MIN I=
              =2441249.3737+0.3207197D*E (J.D.2440500-41600);
               0001!; MIN I=2442697.4039+0.3207144D*E (J.D.
              2441600-43100)  9295!; MIN I=2443459.7476+
              +0.3207216D*E (J.D.2443100-44400)  9297!; MIN I=
              =2444856.8064+0.3207184D*E (J.D.2444400-44900)
               0001!; OCE/SINCE J.D.2444900 - CM.TA./SEE
              TABLE.
              OPMA KPBO ECKA, H MHMMOB  BCO-
              T MAKCMMOB MEHTC./SHAPE OF THE LIGHT CURVE,
              DEPTHS OF MINIMA AND HEIGHTS OF MAXIMA VARY.
TW     LAC    D=0.018P. P VAR. MIN I=2424387.332+3.0374936D*E
              (J.D.2424380-34000)  2389!; MIN I=2434049.593+
              +3.037520D*E (J.D.2434000-36560)  3115!; OCE/
              SINCE J.D.2441500 - CM.TA./SEE TABLE.
TZ     LAC    B PAOHE PACCEHHOO CKOEH/IN THE GERION OF
              THE OPEN CLUSTER NGC 7243.
UW     LAC    HA/DEPTH OF MIN II 0.05M; D=0.028P. P VAR.
              MIN I=2429158.17+5.2902D*E (J.D.2414580-29440)
               1813!; MIN I=2429158.17+5.290000D*E (J.D.
              2429440-35800)  3115!; OCE/SINCE J.D.2436800-
              CM.TA./SEE TABLE.
              BOMOHO BPAEHE H AC/APSIDAL MOTION
              IS POSSIBLE  9300!.
UY     LAC    D=0.022P.
UZ     LAC    P VAR?
VX     LAC    P VAR. MIN=2424791.488+1.0744891D*E (J.D.
              2424700-32400); MIN=2432479.477+1.0744991D*E
              (J.D.2432400-40510); MIN=2440750.971+
              +1.0744881D*E (J.D.2440750-43000)  7552!; OCE/
              SINCE J.D.2443000 - CM.TA./SEE TABLE.
VY     LAC    MIN II 10.6. P VAR? MIN I=2434629.392+1.036245D*E
              (J.D.2424700-39830)  1804!; OCE/SINCE J.D.
              2440080 - CM.TA./SEE TABLE.
WY     LAC    HA KOEAH ECKA C P=850D  A=1.5M HAKA-
              BATC KOEAH C P=50D  A=1M./LIGHT VA-
              RIATIONS WITH P=850D AND A=1.5M ARE SUPERIMPO-
              SED BY VARIATIONS WITH P=50D AND A=1M.
XX     LAC    CM./SEE TZ LAC.
XZ     LAC    P VAR.
AG     LAC    MIN II 14.0.
AR     LAC    MIN II 6.43; MIN II-MIN I=0.5018P; DI=0.045P; DII=
              =0.13P; DII=0.00P. P VAR. MIN I=2426624.378+
              +1.983244D*E (J.D.2415300-26800)  9309!; MIN I=
              =2429535.739+1.9832125D*E (J.D.2426800-36000)
               9312!; MIN I=2437018.414+1.983252D*E (J.D.
              2436000-37500)  0001!; OCE/SINCE J.D.2437500-
              CM.TA./SEE TABLE.
              EMEHT, AHHE B TAE, COEPAT KBAPAT-
              H EH:/THERE IS A SQUARE TERM IN THE ELEMENTS
              GIVEN IN THE TABLE: -5.24D*10**-9*E**2.
              OPMA KPBO ECKA MEHETC; HAAETC C-
              TOPCOHHA BOHA C AMTO O 0.13MV, MP-
              PA B HAPABEH MEHEH A C EPOOM
              - 2.5 OA. CCEOBAH CEKTPA  1816, 9315,
              9316!./SHAPE OF THE LIGHT CURVE VARIES; THERE IS A
              DISTORTION WAVE WITH A UP TO 0.13MV MIGRATING IN THE
              DIRECTION OF DECREASING PHASES WITH P=2.5 YR. SPECT-
              RUM INVESTIGATIONS  1816, 9315, 9316!.
AU     LAC    MIN II 12.2; MIN II-MIN I=0.53P.
AW     LAC    MIN II 11.2.
BH     LAC    H BOOPOA B CEKTPE-KE  OKE./HYD-
              ROGEN LINES IN THE SPECTRUM ARE SHARP AND DEEP  3149!.
BL     LAC    Z=0.07; <B_V>=+1.0. PAK KPBO ECKA/
              LIGHT CURVE GRAPH  6784!.
BM     LAC    EMEHT CPABEB B HTEPBAE/THE ELEMENTS
              ARE VALID IN THE INTERVAL J.D.2425200-26250.
BT     LAC    EMEHT COEPAT KBAPATH EH: -0.0004D*E**2.
              B TAE PBEEHA OXA MAX ECKA. CPEH
              BEHA MEHETC B PEEAX 13.8M-15.2M C P=
              =654D. CPEH AMTA KOPOTKOEPOECKX
              KOEAH - 1.5M. HAAETC CMEHA ABHX 
              BTOPHX MHMMOB ECKA./THERE IS A SQUARE
              TERM IN THE ELEMENTS: -0.0004D*E**2. EPOCH OF MAX
              BRIGHTNESS IS GIVEN IN THE TABLE. MEAN BRIGHTNESS VA-
              RIES IN THE RANGE 13.8M-15.2M WITH P=654D. MEAN
              AMPLITUDE OF THE SHORTPERIODICAL VARIATIONS IS - 1.5M.
              THERE OCCUR CHANGES OF PRIMARIES AND SECONDARIES MI-
              NIMA INTO EACH OTHER.
BU     LAC    HA OCHOBHOE KOEAHE HAKABATC BOH C
              BOMOHM EPOOM - 200D./THE MAIN VARIATION
              IS SUPERIMPOSED BY WAVES WITH A POSSIBLE PERIOD
              - 200D.
CG     LAC    MIN II 14.0.
CM     LAC    MIN II 8.53; DII=0.12P.
CN     LAC    MIN II 12.6. B PAOHE PACCEHHOO CKOEH
              NGC 7209. HE EH CKOEH./IN THE REGION OF THE
              OPEN CLUSTER NGC 7209. NOT MEMBER OF THE CLUSTER.
CO     LAC    MIN II 10.79. HAAETC BEHE H AC C
              P=42.3 OA. EMEHT, PBEEHHE B TAE,
              COEPAT EPOECK EH:/APSIDAL MOTION WITH
              P=42.3 YR IS OBSERVED. THERE IS A PERIODIC TERM IN
              THE ELEMENTS GIVEN IN THE TABLE: -0.0133D COS(157.7G+
              +0.0359G E).
              MIN II=2427534.8439+1.5422075D*E+0.0133D COS(157.7G+
              +0.0359G*E).
CS     LAC    MIN II 9.4.
CZ     LAC    DS=1. P VAR. MAX=2432878.234+0.43210346D*E
              (J.D.2428700-39400)  1442!; MAX=2443081.309+
              +0.4319850D*E (J.D.2439400-43100)  5839!; MAX=
              =2444080.122+0.432114D*E (J.D.2443800-44100)
               9009!; OCE/SINCE J.D.2445100 - CM.TA./SEE
              TABLE.
DD     LAC    VB A (B 9.2M, 69", 16G).  P VAR. MAX=2421914.178+
              +0.19309018D*E-0.001798D*10**-8*E**2 (J.D.2421400-
              37600)  5711!; OCE/SINCE J.D.2443000 - CM.
              TA./SEE TABLE.
              COACHO  9337!, OHOBPEMEHHO HAATC -
              CA CO CEM EPOAM (B CKOKAX-COOT-
              BETCTBE HAEH AB):/ACCORDING TO  9337!
              SIMULTANEOUSLY THE PULSATIONS WITH THE FOLLOWING PE-
              RIODS ARE OBSERVED (THE CORRESPONDING AB VALUES ARE
              GIVEN IN THE BRACKETS): P1=0.193082D (0.080M), P2=
              =0.197382D (0.034M), P3=0.182115D (0.020M), P4=
              =0.187438D (0.016M), P5=0.095109D (0.010M), P6=
              =0.23583D (0.008M). A VAR; 0.04M=<A=<0.12M.
DE     LAC    DS=5. P VAR. MAX=2428807.130+0.2536940D*E (J.D.
              2427000-33000); MAX=2433005.766+0.2536929D*E
              (J.D.2433000-39100)  3378!; OCE/SINCE J.D.
              2442000 - CM.TA./SEE TABLE.
DF     LAX     A/H!=0.2.
DG     LAC    P VAR. MIN=2426266.355+2.206435D*E (J.D.2426200-
              40000)  4961!; OCE/SINCE J.D.2440000 - CM.TA./
              SEE TABLE.
DH     LAC    P VAR. MAX=2418240+284.8D*E (J.D.2418000-
              27350); OCE/SINCE J.D.2427300 - CM.TA./SEE
              TABLE.
DO     LAC    COACHO/ACCORDING TO  0085!, EA.
EG     LAC    P>50D?  5386!.
EM     LAC    MIN II 13.09.
EN     LAC    VB A (B 11.32MV, 27", 345G; C 9.0MV, 62", 48G); SB1
              (PORB=12.0968D). ATMEHHA CCTEMA C CP-
              M ABHM KOMOHEHTOM TA BCEP. HA
              MIN I 0.05MB. MIN I=2444909.4339+12.096816D*E;
              D=0.015P, D=0.000P. OHOBPEMEHHO HAATC
              CA C EPOAM P1=0.169170D, P2=0.170770D,
              P3=0.181692D  9346!. COOTBETCTBE AMT
              CA MEHTC. HE PBOTC HAEH
              AMT B CCTEME B:/ECLIPSING SYSTEM WITH A
              PULSATING PRIMARY COMPONENT OF BCEP TYPE. DEPTH OF
              MIN I 0.05MB. MIN I=2444909.4339+12.096816D*E;
              D=0.015P, D=0.000P. SIMULTANEOUSLY PULSATIONS ARE
              OBSERVED WITH THE PERIODS P1=0.169170D, P2=0.170770D,
              P3=0.181692D  9346!. THE CORRESPONDING AMPLITUDES
              OF PULSATIONS VARY. THE VALUES OF THE AMPLITUDES IN
              B SYSTEM ARE AS FOLLOWS: A1=0.046M, A2=0.024M,
              A3=0.022M (1952-1965); A1=0.016M, A2=0.010M,
              A3=0.014M (1977); A1=0.010M, A2=0.014M, A3=0.023M
              (1980-81). 0.01M=<A=<0.11M.
EO     LAC    MIN II 12.9; MIN II-MIN I=0.485P.
EP     LAC    HA/DEPTH OF MIN II 0.04M.
ER     LAC    HA/DEPTH OF MIN II 0.05M:.
ES     LAC    MIN II 11.6; MIN II-MIN I=0.57P. BOMOHO BPAE-
              HE H AC:/APSIDAL MOTION IS POSSIBLE: MIN II=
              =2433582.95+4.459451D*E  9347!.
EV     LAC    VB A (B 12.74MB, 10", 260G, 1949); MU ALFA=-0.065S,
              MU DELTA=-0.46". TEMH CTHK/DARK COMPANION (A=
              =0.0206", P=45 YR, E=0.5)  9348!.
              B 1979 . HAAC CHCOAHE KOEAH
              ECKA B PEEAX 10.20M-10.27MV: MIN=
              =2444037.576+4.378D*E  9349!. B 1974-76 . TA-
              KA EPOHOCT HE HAAAC  9350!./IN 1979
              SINUSOIDAL LIGHT OSCILLATIONS WERE OBSERVED IN THE
              RANGE 10.20M-10.27MV: MIN=2444037.576+4.378D*E
               9349!. IN 1974-76 SUCH PERIODICITY WAS NOT OBSERVED
               9350!.
EW     LAC    BOMOH TAKE HEPAAHE CA C P=
              =0.7D-0.8D/NON-RADIAL PULSATIONS WITH P=0.7D-0.8D
              ARE ALSO POSSIBLE  9351, 9352!.
EX     LAC    D=0.050P.
FQ     LAC    A VAR; P VAR. AHHE B TAE EMEHT CPABE-
              B B HTEPBAE/ELEMENTS GIVEN IN THE TABLE ARE
              VALID IN THE INTERVALE J.D.2427950-31700.
FU     LAC    D=0.013P.
GS     LAC    MIN II 15.2.
GX     LAC    MIN II 10.23.
HK     LAC    SB1 (PORB=24.4284D  9355!).
HM     LAC    CM./SEE ER LAC.
HN     LAC    MIN II 14.7.
HR     LAC    MIN II 14.3.
HT     LAC    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 7209.
HW     LAC    MIN II 14.8.
HX     LAC    MIN II 14.8.
HZ     LAC    MIN II 15.0.
IM     LAC    MIN II 13.2.
IN     LAC    E?
IP     LAC    MIN II 14.0.
IR     LAC    MIN II 15.4; D=0.03P.
IT     LAC    P VAR.
IU     LAC    MIN II 13.5.
IY     LAC    BOMOEH EKT AKO./BLAZHKO EFFECT?
IZ     LAC    MIN II 12.7.
KO     LAC    MIN II 14.7.
KP     LAC    P<1D.
KR     LAC    MIN II 15.8; DII=0.05P.
KS     LAC    HA/DEPTH OF MIN II 0.03M.
KU     LAC    CM./SEE KS LAC.
LU     LAC    MIN II 15.32.
LW     LAC    D=0.03P. HA/DEPTH OF MIN II 0.03M?
LY     LAC    MIN II 12.6.
LZ     LAC    MIN II 12.5.
MO     LAC    D=0.04P. CM./SEE ER LAC.
MP     LAC    MIN II 12.5.
MV     LAC    MIN II 15.0.
MZ     LAC    MIN II 12.1; MIN II-MIN I=0.713P. MIN II=
              =2433872.702+3.158719D*E. B TAE AH E-
              MEHT  MIN I./ELEMENTS FOR MIN I ARE GIVEN IN
              THE TABLE.
NN     LAC    D=0.02P. CEBEPO-AAH (OHO OEE PK)
              KOMOHEHT TECHO AP. PBEEH PEE -
              MEHEH CMMAPHOO ECKA./NP (USUALLY BRIGH-
              TER) COMPONENT OF A CLOSE PAIR. THE RANGE OF COM-
              BINED BRIGHTNESS IS GIVEN IN THE TABLE.
NO     LAC    CM./SEE KS LAC.
NR     LAC    MIN II 13.4. O-AAH (OEE PK) KOMOHEHT
              TECHO AP. AH PEE MEHEH CMMAPHOO
              ECKA./SP (BRIGHTER) COMPONENT OF A CLOSE PAIR. THE
              RANGE OF COMBINED BRIGHTNESS IS GIVEN IN THE TABLE.
NU     LAC    EW?
NW     LAC    MIN II 13.9. TECHA BOHA C PABHM O ECK
              KOMOHEHTAM B MIN ECKA. AH PEE MEHE-
              H CMMAPHOO ECKA./CLOSE BINARY, THE COMPO-
              NENTS OF WHICH ARE EGUAL IN BRIGHTNESS AT MINIMUM
              LIGHT. THE RANGE OF COMBINED BRIGHTNESS IS GIVEN IN
              THE TABLE.
OO     LAC    MIN II 12.8.
OV     LAC    150D<=P<=200D.
OX     LAC    CM./SEE EP LAC.
PP     LAC    MIN II 12.0.
PT     LAC    MIN II 15.4.
PZ     LAC    CM./SEE TZ LAC.
QQ     LAC    CM./SEE TZ LAC.
QU     LAC    CM./SEE EP LAC.
V335   LAC    MIN II 15.8.
V338   LAC    B PAOHE PACCEHHOO CKOEH./IN THE REGION OF
              THE OPEN CLUSTER IC 1434.
V339   LAC    P=3.4084964D?
V340   LAC    MIN II 12.4; MIN II-MIN I=0.762P; MIN II=2432858.521+
              +19.943102D*E. B TAE AH EMEHT  MIN I./
              ELEMENTS FOR MIN I ARE GIVEN IN THE TABLE.
V342   LAC    MIN II 12.9.
V343   LAC    MIN II-MIN I=0.57P. HA/DEPTH OF MIN II 0.03M:.
V344   LAC    MIN II 13.0. MIN I=2433873.5784+0.39222768D*E (J.D.
              2432800-35800); OCE/SINCE J.D.2445200-CM. TA./
              SEE TABLE.
V345   LAC    MIN II 11.6; MIN II-MIN I=0.340P; DII=0.040P; DII=
              =0.014P. BOMOHO BEHE H AC./APSI-
              DAL MOTION IS POSSIBLE.
V347   LAC    VB.
V350   LAC    VB A (B 9.7M, 66", 94G); SB 1 (P=17.755D  9356!).
              MIN II 6.45  7468!. CPEH BEHA MEHETC. CM.
              TAKE  8933!./MEAN MAGNITUDE VARIES. SEE ALSO
               8933!.
V355   LAC    CEBEPH KOMOHEHT BOHO./NORTHERN COMPONENT
              OF A PAIR.
V360   LAC    SB 2 (P=10D  9357!). MIN II 5.93.
V362   LAC    VB A (B 13.2M, 1.8", 49G).
V363   LAC    VB A (B 11.3M, F6 III-V:, 6.3", 325G).
V364   LAC    MIN II 9.15; MIN II-MIN I=0.52P; DI=0.003P, DII=
              =0.077P, DII=0.009P.
R      LEO    P VAR. MAX=2385112+312.43D*E (J.D.2385100-
              2402500); MAX=2402929+314.33D*E (J.D.2402500-
              11500); MAX=2411416+308.93D*E (J.D.2411500-
              16500); MAX=2416984+317.84D*E (J.D.2416500-
              22500); MAX=2423328+312.75D*E (J.D.2422500-
              27000); MAX=2427081+307.40D*E (J.D.2427000-
              30000); MAX=2437337+312.13D*E (J.D.2430000-
              37500); OCE/SINCE J.D.2437500-CM. TA./SEE
              TABLE.
              SIO, H2O, OH MAEP/MASER.
S      LEO    P VAR. MAX=2420654+189.24D*E (J.D.2420200-
              26100); MAX=2426142+185.92D*E (J.D.2426100-
              28100); OCE/SINCE J.D.2428100-CM. TA./SEE
              TABLE.
T      LEO    SB 1 (PORB=0.05881873D  9304!).
V      LEO    H2O MAEP/MASER.
W      LEO    P VAR. MAX=2434651+385.41D*E (J.D.2409500-
              35000); OCE/SINCE J.D.2437500-CM. TA./SEE
              TABLE.
              OH MAEP/MASER.
Y      LEO    P VAR. MIN=2422372.520+1.6860978D*E (J.D.2418000-
              23500)  2389!; MIN=2422372.5368+1.68607314D*E
              (J.D.2423500-38600)  9307!; OCE/SINCE J.D.
              2438600-CM. TA./SEE TABLE.
              EMEHT, PBEEHHE B TAE, COEPAT EPO-
              ECK EH:/THERE IS PERIODIC TERM IN THE ELE-
              MENTS GIVEN IN THE TABLE:+0.00375D*SIN(0.21487G*E+
              +141.7G). HA/DEPTH OF MIN II 0.1M IR.
RR     LEO    DS=7.1. P VAR. MAX=2430440.3385+0.45238172D*E+
              +1.963D*10**-10*E**2 (1898-1977)  8299!; OCE/SINCE
              J.D.2441400-CM. TA./SEE TABLE.
RT     LEO    MIN II 10.5.
RW     LEO    P VAR. O/BEFORE J.D.2440800 MIN=2424993.458+
              +1.6825365D*E  3115!; OCE/SINCE J.D.2440800-
              CM. TA./SEE TABLE.
RX     LEO    DS=6.8.
SS     LEO    P VAR. MAX=2415485.723+0.62633242D*E (J.D.
              2414000-22000)  0752!; OCE/SINCE J.D.2422000-
              CM. TA./SEE TABLE.
               FE/H!=-1.59.
ST     LEO    (K-B)2=0.08.
SZ     LEO    P VAR. O/BEFORE J.D.2442500 MAX=2425331.400+
              +0.5340833D*E  4157!; OCE/SINCE J.D.2442500-
              CM. TA./SEE TABLE.
              OPMA KPBO ECKA VAR?/LIGHT CURVE SHAPE VAR?
TU     LEO    B MIN ECKA:/IN LIGHT MINIMUM:+0.22<=B-V<=+0.56,
              U-B=-0.08, J=14.05M, K=12.91M.
              OHA OCTOBEPHA BCKA./SINGLE RELIABLE OUTBURST.
TV     LEO    P VAR. MAX=2419852.318+0.6728362D*E (J.D.
              2419000-28000)  0001!; OCE/SINCE J.D.2437000-
              CM. TA./SEE TABLE.
              (K-B)2=-0.01.
TX     LEO    VB A (B 7.8M, 2", 157G, 1971); BOHA O AHHM
              OKPT HO:/A BINARY ACCORDING TO LUNAR OCCUL-
              TATION DATA:RO=0.0005".
              AH PEE MEHEH CMMAPHOO ECKA./THE
              RANGE OF COMBINED BRIGHTNESS IS GIVEN.
              MIN II 5.69; DII=0.19P; MIN II-MIN I=0.550P.
TY     LEO    EMEHT TPET OTBEPEH./ELEMENTS NEED
              CONFIRMATION.
UU     LEO    MIN II 11.5. P VAR. OCE/SINCE J.D.2430000-CM.
              TA./SEE TABLE.
UV     LEO    MIN II 9.49; D=0P014. P VAR. O/BEFORE J.D.
              2434000 MIN I=2425574.302+0.60008516D*E  7554!;
              OCE/SINCE J.D.2434000-CM. TA./SEE TABLE.
UX     LEO    MIN II 10.4. MOMEHT MHMMOB BBS.AG POTBO-
              PEAT EMEHTAM B TAE./MOMENTS OF MIN BY
              BBSAG CONTRADICT THE TABULATED ELEMENTS.
UZ     LEO    MIN II 10.12. P VAR, KBAPATH EH:/NONLINEAR
              TERM:+2.8D*10**-12*E**2.
XX     LEO    MIN II 11.4. EPO TPEET TOHEH./PERIOD
              SHOULD BE CHECKED.
XY     LEO    MIN II 9.80. P VAR. MIN=2435195.66306+0.2841091D*E
              (J.D.2434000-36500)  3392!; MIN=2437376.465+
              +0.28409592D*E (J.D.2436500-40000)  0001!; MIN=
              =2441005.5364+0.28410727D*E (J.D.2441000-44000)
               9084!; OCE/SINCE J.D.2444000-CM. TA./SEE
              TABLE.
              OPMA KPBO ECKA/THE LIGHT CURVE SHAPE VAR.
XZ     LEO    MIN II 11.1.
AB     LEO    AHA OXA MIN./EPOCH OF MIN IS GIVEN.
              COACHO/ACCORDING TO  1853!, MAX=2428880+
              +103.2D*E (J.D.2414600-19000, 2428000-31600);
              B POE BPEM K/DURING OTHER TIME INTERVALS
              CYCLES 75D-125D.
AD     LEO    MU=0.49", P=265G; PI=0.20". PEHTEHOBCK  PA-
              OCTOHK./X-RAY AND RADIO SOURCE.
              ACTPOMETPECKA BOHA?/ASTROMETRIC BINARY?
AF     LEO    H2O MAEP/MASER.
AM     LEO    VB A (B 10.64M, 11", 270G). MIN II 9.83.
AP     LEO    MIN II 9.88. P VAR. MIN=2414986.868+0.430350D*E
              (J.D.2414700-18600); OCE/SINCE J.D.2418600-
              CM. TA./SEE TABLE.
              OPMA KPBO ECKA/LIGHT CURVE SHAPE VAR.
AQ     LEO    EMEHT  OCHOBHOO TOHA CA (P0) CM.
              TA./ELEMENTS FOR FUNDAMENTAL MODE PULSATIONS (P0)
              SEE TABLE.
               EPBOO OEPTOHA:/FOR THE FIRST OVERTONE: P1 VAR?;
              P1=0.4101369D (1929-1969); P1=0.410130D (1957-
              1969); B HTEPBAE/DURING 1973-1975 MAX1=
              =2441766.486+0.4101487D*E. DM0=0.23M, DM1=0.46M.
AU     LEO    VR=+7545 KM/S. EPEMEHHOCT COMHTEHA./VARIA-
              BILITY IS DOUBTFUL.
BB     LEO     FE/H!=-1.32.
BL     LEO    MIN II14.4. P VAR. OCE/SINCE J.D.2442000-CM.
              TA./SEE TABLE.
BV     LEO    MIN II 16.1.
BW     LEO    MIN II 15.4.
BX     LEO     FE/H!=-1.23.
BZ     LEO    MIN II 15.8.
CD     LEO    OPMA KPBO ECKA/LIGHT CURVE SHAPE VAR.
CE     LEO    MIN II 12.5. P VAR? MOMEHT MHMMOB BBS AG
              POTBOPEAT EMEHTAM, PBEEHHM B TA-
              E./MIN BY BBSAG CONTRADICT THE TABULATED ELE-
              MENTS.
CN     LEO    MU=4.7", P=235G; PI=0.41". MK PEHTEHOBCK
              CTOHK, PAOCTOHK./SOFT X-RAY SOURCE, RADIO
              SOURCE.
CW     LEO    EBA OOOKA 6"*4"./DUST ENVELOPE, 6"*4".
              MOEKPHA PAOMCC:/MOLECULAR RADIOEMIS-
              SION:SIO, SIS, HCN, HC3N, CO, H2O, NH3, ETC.
              OPA B AX I O 24%./POLARIZATION IN I
              BAND UP TO 24%.
CX     LEO    VB A (B 12.3M, 132G); SB (PORB=12685.4D).
CY     LEO    MU=0.307", P=141.3G; PI=0.022". BHE BCEK/
              OUTSIDE FLARES DM<=0.036M; P=600S, 822S, 1638S
               6209!.
              HAAAC OHA CHA BCKA C DM=0.61M B
              CHX AX POOTEHOCT 10 MH  6141!,
              KOTOP HEKOTOPE ABTOP CBBAT C HAEM
              KPACHOO BCXBAEO KOMOHEHTA./A SINGLE
              STRONG FLARE WITH DM=0.61M IN BLUE LIGHT OF 10 MIN
              DURATION WAS OBSERVED  6141!,  WHICH IS ATTRIBUTED BY
              SEVERAL AUTHORS TO THE PRESENCE OF A RED FLARING COM-
              PANION.
DE     LEO    P=1.2D-2.0D?
DG     LEO    VB B (A 6.6M, A 8IV, SB 2, PORB=4.15D; B 6.9M, 0.271",
              211.2G, 1980, PORB-200YR). AH PEE ME-
              HEH CMMAPHOO ECKA./ THE RANGE OF THE COM-
              BINED BRIGHTNESS IS GIVEN.
DH     LEO    SB 1, PORB=1.070354D.
DK     LEO    MU ALFA=-0.097", MU DELTA=-0.214".
R      LMI    SIO, H2O, OH MAEP/MAZER.
T      LMI    MIN II 10.97. P VAR. MIN I=2420573.698+3.019889D*E
              (J.D.2420200-25000); MIN I=2423856.323+
              +3.0199336D*E (J.D.2423800-35500); OCE/SINCE
              J.D.2438400-CM. TA./SEE TABLE.
U      LMI    1M<=A<=3.3M. EPOHOCT HOA HAPAETC/
              PERIODICITY SOMETIMES BREAKS DOWN.
V      LMI    DS=5.7.
Y      LMI    P VAR. MAX=2428636.322+0.52443938D*E+0.0597D*
              *SIN(0.0657G*E+27.2G) (J.D.2425250-28500); MAX=
              =2428636.348+0.5244564D*E (J.D.2428500-30000)
               1856!; B TAE PBEEH CPEHE EMEHT
               HTEPBAA J.D.2432200-38900, B KOTOPOM E-
              PO MEHC C KOM-2100D/MEAN ELEMENTS
              FOR INTERVAL J.D.2432200-38900 ARE GIVEN IN THE
              TABLE; IN THIS INTERVAL THE PERIOD CHANGED WITH THE
              CYCLE OF-2100D.
              EKT AKO C EPOOM 33.4D/BLAZHKO EFFECT
              WITH THE PERIOD 33.4D  1856!; 07M<=A<=1.9M, 0.19P<=
              <=M-M<=0.44P.
RT     LMI    MIN II 11.7.
RU     LMI    OCAHE CEKTPA/SPECTRUM DESCRIPTION  9326!.
RW     LMI    VB A (B 15.5M B, 9", 10G). 0.3M-2.6M K, 7.64M-10.71M,
              9.7M-14.6M R, 14.1M-18.1M B, 14.8M-18.6M U. CPE-
              H ECK MEHETC. AOEBA OKOOBEHA
              OOOKA. MCC CO. OCAHE CEKTPA  9327!./
              MEAN BRIGHTNESS VARIES. GASEOUS-DUST CIRCUMSTEL-
              LAR ENVELOPE. CO EMISSION. SPECTRUM DESCRIPTION
               9327!.
RY     LMI    VB A (B 16.1M, DM2, 15", 126G); MU=0.14", P=264G.
              P0=215.197388S, P0=5.6S*10**-14/S, A0=0.0440M;
              P1=304.4S, A1=0.0150M; P2=271.0S, A2=0.0134M;
              P3=107.6S, A3=0.0032M; P4=126.2S, A4=0.0028M;
              P5=119.8S, A5=0.0026M. CPEH ECK MEHETC
              HA 0.05M./MEAN BRIGHTNESS VARIES BY 0.05M.
R      LEP    P VAR. MAX=2398883+436.44D*E (J.D.2398000-
              2412000); MAX=2412849+418.04D*E (J.D.2412000-
              23000); MAX=2423300+441.38D*E (J.D.2423000-
              36000); OCE/SINCE J.D.2436000-CM. TA./SEE
              TABLE.
              A VAR; 5.5M<=MAX<=9.5M (BOMOH EPO O-
              E 40 ET/POSSIBLE PERIOD IS MORE THAN 40 YEARS
               3402!).
S      LEP    CPEH BEHA MEHETC C KOM 890D./MEAN
              MAGNITUDE VARIES WITH THE CYCLE OF 890D. H2O MA-
              EP/MASER.
T      LEP    SIO MAEP/MASER.
U      LEP    P VAR. MAX=2425084.431+0.58147098D*E (J.D.
              2411000-25090); MAX=2425084.431+0.58147377D*E
              (J.D.2425080-37700)  3403!; OCE/SINCE J.D.
              2436600-CM. TA./SEE TABLE.
              DS=8.5; (K-B)2=0.00.
V      LEP    MIN II 9.9.
Z      LEP    MIN II 12.0:.
RR     LEP    MIN II 10.4.
RS     LEP    MIN II 9.96.
RU     LEP    P VAR?
RZ     LEP    S 4/4.
SS     LEP    SB 2 (PORB=258.2D  9363!).
SY     LEP    VB A (B 15.2M: V, 18", 270G).
S      LIB    P VAR. MAX=2405692+192.14D*E (J.D.2402700-
              24000); MAX=2424141+194.74D*E (J.D.2424000-
              30500); MAX=2431900+190.34D*E (J.D.2430500-
              37200); MAX=2439203+197.61D*E (J.D.2437200-
              39300); OCE/SINCE J.D.2441000-CM. TA./SEE
              TABLE.
              B TAE PBEEHO CPEHEE HAEHE EPOA./
              MEAN VALUE OF THE PERIOD IS GIVEN IN THE TABLE.
              A VAR (1.8M<=A<=5M).
W      LIB    P VAR. MAX=2412272+203.76D*E (J.D.2412000-
              28500); MAX=2428573+201.48D*E (J.D.2428500-
              34000); OCE/SINCE J.D.2434000-CM. TA./SEE
              TABLE.
X      LIB    P VAR. MAX=2423500+165.75D*E (J.D.2413000-
              25000); OCE/SINCE J.D.2425000-CM. TA./SEE
              TABLE.
Y      LIB    P VAR. MAX=2413452+275.7D*E (J.D.2413400-
              22000); MAX=2422273+272.5D*E (J.D.2422000-
              28000)  0458!; MAX=2434921+277.04D*E (J.D.
              2428000-35000); OCE/SINCE J.D.2435000-CM.
              TA./SEE TABLE.
Z      LIB    P VAR. MAX=2417736+294.5D*E (J.D.2407100-17800);
              OCE/SINCE J.D.2424400-CM. TA./SEE TABLE.
RR     LIB    P VAR. MAX=2409699+277.4D*E (J.D.2409600-
              15600); MAX=2416345+273.2D*E (J.D.2416300-
              19700); MAX=2421027+278.6D*E (J.D.2421000-
              27150)  0458!; OCE/SINCE J.D.2427150-CM. TA./
              SEE TABLE.
RS     LIB    P VAR. MAX=2413396+217.2D*E (J.D.2413300-
              20000); MAX=2420110+219.6D*E (J.D.2420000-
              27500)  0458!; MAX=2429078+215.6D*E (J.D.2427500-
              35000); MAX=2438196+219.9D*E (J.D.2435000-
              42600); OCE/SINCE J.D.2441700-CM. TA./SEE
              TABLE.
RT     LIB    P VAR. MAX=2413776+254.21D*E (J.D.2413000-
              19000); OCE/SINCE J.D.2419000-CM. TA./SEE
              TABLE.
RU     LIB    P VAR. MAX=2413363+312.0D*E (J.D.2413300-
              16200); MAX=2416807+322.5D*E (J.D.2416800-
              21000); MAX=2421309+317.0D*E (J.D.2421300-
              24200); MAX=2424804+311.5D*E (J.D.2424800-
              29800)  0458!; MAX=2434909+319.9D*E (J.D.2429800-
              35000); OCE/SINCE J.D.2437700-CM. TA./SEE
              TABLE.
RV     LIB    MIN II 9.44.
RX     LIB     A/H!=-0.5. P VAR. MAX=2430913.6+24.950D*E
              (J.D.2425000-36300)  0266!; OCE/SINCE J.D.
              2436300-CM. TA./SEE TABLE.
SS     LIB    MIN II 10.8; D=0.030P.
ST     LIB    VB A (B 14M, 14", 0G).
TV     LIB    DS=2.5.
TY     LIB    D=0.019P.
UW     LIB     FE/H!=-0.25.
VV     LIB    P VAR. MAX=2424268.474+0.4781418D*E (J.D.
              2419800-2425000); OCE/SINCE J.D.2425000-CM.
              TA./SEE TABLE.
VW     LIB    HAEH B  0293! POTBOPEAT EMEHTAM,
              PBEEHHM B TAE./OBSERVATIONS GIVEN IN
               0293! CONTRADICT THE ELEMENTS GIVEN IN THE TABLE.
VY     LIB    P VAR?  3506!.DS=6.
VZ     LIB    MIN II 10.55; DI=0.000P; DII=0.005P. P VAR. MIN I=
              =2429022.227+0.358053D*E (J.D.2428600-30400)
               9368!; MIN I=2430899.223+0.358448D*E (J.D.
              2430400-32400)  2532!; OCE/SINCE J.D.2444330-
              CM. TA./SEE TABLE.
YZ     LIB    MIN II 12.9.
AA     LIB    P VAR? EMEHT OBETBOPT HAEHM B
              HTEPBAE/THE ELEMENTS ARE VALID IN THE INTERVAL
              J.D.2427800-29600.
AP     LIB    Z=0.0486.
AQ     LIB     FE/H!=-0.60.
BT     LIB    MIN II 12.3.
CG     LIB     FE/H!=-1.82. P VAR. MAX=2438592.287+
              +0.3068674D*E (J.D.2427800-39600)  7557!; OCE/
              SINCE J.D.2439600-CM. TA./SEE TABLE.
EH     LIB    DS=0. 9.35M<=MAX<=9.49M V; MAX (A)=2442162.556+
              +0.273778D*E  9336!.
ES     LIB    MIN II 7.33.
EU     LIB    70D<=P<=90D.
FI     LIB    90D<=P<=110D.
FS     LIB    OH MCC/EMISSION.
FX     LIB    OCAHE CEKTPA/SPECTRUM DESCRIPTION  6167,
              9371!.
DELTA  LIB    VB A (B 11.3M, 9", 351G; C 12.80M, 67", 90G); MIN II
              4.98. P VAR?
S      LUP    VB A (B=X LUP, 13", 176G). P VAR. MAX=2411950+
              +347.81D*E (J.D.2411950-14000); MAX=2414040+
              +339.31D*E (J.D.2414000-19000); MAX=2419135+
              +345.12D*E (J.D.2419000-26000); MAX=2426038+
              +336.60D*E (J.D.2426000-29500); MAX=2429743+
              +345.15D*E (J.D.2429500-35000); OCE/SINCE J.D.
              2437600-CM. TA./SEE TABLE.
X      LUP    VB B (CM./SEE S LUP).
Y      LUP    P VAR. MAX=2424691+408.15D*E (J.D.2423000-
              25500); MAX=2425503+394.81D*E (J.D.2425500-
              30250); MAX=2430641+407.75D*E (J.D.2430250-
              35000); OCE/SINCE J.D.2437900-CM. TA./SEE
              TABLE.
RU     LUP    BPEMEHAM MEHETC KBAEPOECK:/SOME-
              TIMES VARIES QUASIPERIODICALLY: P1=3.5457D, P2=
              =3.8375  2412!. H2O MAEP/MASER.
RY     LUP    KBAEPOHOCT:/QUASIPERIODICITY: P=3.7609D
               9366!.
SX     LUP    MIN II 11.8.
UX     LUP     A/H!=-0.9. P VAR. P=16.2403D (J.D.2411526-
              14040); P=16.2065D (J.D.2414040-24016); P=
              =16.2492D (J.D.2424016-25638); P=16.1794D (J.D.
              2425638-26449); P=16.2241D (J.D.2426449-29693)
               5387!.
VV     LUP    K CTHK HA CEBEPE./CLOSE NORTHERN COMPA-
              NION.
VZ     LUP    P VAR? OPMA KPBO ECKA/LIGHT CURVE SHAPE
              VAR?
CX     LUP    MIN II 12.8.
CY     LUP    BCOKE MAX KAE 360D; A 80D EPE HM-
              HAOEE OKE MIN./HIGH MAX EVERY 360D, ES-
              PECIALLY FAINT MIN 80D BEFORE THESE HIGH MAX.
DG     LUP    MIN II 15.1.
EL     LUP    VB.
ER     LUP    P2=140D.
FK     LUP    MIN II 10.7:.
FR     LUP    OK/DEEP MIN II.
FT     LUP    MIN II 9.98. DI=0.025P?, DII>=0.066P. P VAR. O/
              BEFORE J.D.2439300 MIN I=2427987.310+0.470089D*E
               3948!; OCE/SINCE J.D.2445000-CM. TA./SEE
              TABLE.
              BCE HAEH XOPOO PECTABTC TAKE E-
              MEHTAM:/ALL THE OBSERVATIONS ARE WELL REPRESENTED
              ALSO BY THE ELEMENTS: MIN I=2445061.834+
              +0.470083D*E-0.114D*10**-9*E**2  9360!.
              OPMA KPBO ECKA/LIGHT CURVE SHAPE VAR?
FV     LUP    MIN II 11.2.
GG     LUP    MIN II 5.8.
GN     LUP    VB A (B 10.2M VIS, 10", 98G).
GO     LUP    CPABHTEHO KOPOTK P./RELATIVELY SHORT P.
GW     LUP    B TEMHO TMAHHOCT/IN THE DARK NEBULA BAR-
              NARD 228.
HK     LUP    B-V:+1.23, +1.46.
HL     LUP    2U 1543-47.
HM     LUP    B-V:+1.12.
HN     LUP    B-V:+1.55, +1.68.
HO     LUP    B-V:+0.70, +0.81.
ALFA   LUP    VB A (B 14.0M, 27.6", 232G, 1901). CTOHK M-
              KOO PEHTEHOBCKOO EH./SOFT X-RAY
              SOURCE.
              P2=3.145D BOMOEH/IS POSSIBLE  8417!.
DELTA  LUP    MEHEE BEPOTH BAPAHT EMEHTOB:/LESS PRO-
              BABLE VARIANT OF ELEMENTS: MAX=2441045.160+
              +0.14273*E.
R      LYN    S 4/5E-S 6/6-.
S      LYN    VB A (B 14M, 12.6", 155G). P VAR. MAX=2414564+
              +300.26D*E (J.D.2414500-27400); MAX=2434241+
              +294.42D*E (J.D.2427400-35100); MAX=2440225+
              +300.44D*E (J.D.2435100-40220); OCE/SINCE J.D.
              2440220-CM. TA./SEE TABLE.
T      LYN    P VAR. MAX=2425012+419.0D*E (J.D.2412800-34700);
              OCE/SINCE J.D.2434700-CM. TA./SEE TABLE.
U      LYN    H2O, OH MCC/EMISSION. P VAR. MAX=2417168+
              +440.3D*E (J.D.2417100-26000)  0458!; MAX=
              =2435908+432.05D*E (J.D.2426000-36000); MAX=
              =2439898+447.1D*E (J.D.2436000-40000); OCE/
              SINCE J.D.2440000-CM. TA./SEE TABLE.
V      LYN    K 55D  87D CMEHT P PA. CPEH
              BEHA MEHETC./CYCLES 55D AND 87D REPLACE
              ONE ANOTHER. MEAN BRIGHTNESS VARIES.
Y      LYN    SB.
RR     LYN    VB A (B 10M, 50"). MIN II 5.90; MIN II=2438051.3115+
              +9.945074D*E; E=0.081; MIN II-MIN I=0.45P (J.D.
              2437700).
RW     LYN     FE/H!=-1.37.
RZ     LYN    MIN II 10.8.
SW     LYN    MIN II 9.65; DI=0.038P. P VAR. MIN I=2425643.323+
              +0.6440661D*E (J.D.2425640-35850)  2742!; MIN I=
              =2438795.8016+0.6440520D*E (J.D.2438380-840)
               9387!; MIN I=2440614.0107+0.6440729D*E (J.D.
              2439500-40620)  0001!; MIN I=2442786.4493+
              +0.6440677D*E (J.D.2440650-42790)  7292!; OCE/
              SINCE J.D.2442780-CM. TA./SEE TABLE.
SX     LYN    MIN II 10.1. P VAR. MIN I=2428636.375+2.0225615D*E
              (J.D.2427400-34700)  0519!; MIN I=2442561.424+
              +2.0225172D*E (J.D.2442400-44000); OCE/SINCE
              J.D.2444000-CM. TA./SEE TABLE.
SZ     LYN    SB (PORB=1146D, E=0.26  9388!). DS=0. EMEHT
              COEPAT EPOECK EH:/THERE IS A PERIO-
              DICAL TERM IN THE ELEMENTS:-0.00573D COS 2PI (EP0/P1+
              +0.007); P0=0.120534920D, P1=1150D.
              AMTA  OPMA KPBO ECKA MEHTC/AMP-
              LITUDE AND SHAPE OF THE LIGHT CURVE VARY.
TT     LYN    DS=7.
TV     LYN     FE/H!=-0.99.
TW     LYN    DS=10. P VAR. MAX=2418676.804+0.4817201D*E (J.D.
              2418670-20155); MAX=2420155.685+0.4816929D*E
              (J.D.2420155-27480); MAX=2427479.359+
              +0.4817481D*E (J.D.2427480-28630); MAX=
              =2428627.310+0.4818529D*E (J.D.2428620-37800)
               2819!. OCE/SINCE J.D.2445000-CM. TA./SEE
              TABLE.
TZ     LYN    AHA OXA MIN ECKA./EPOCH OF MIN BRIGHTNESS
              IS GIVEN.
UU     LYN    MIN II 11.82.
UV     LYN    MIN II 9.78.
UZ     LYN    VR VAR (P=0.065D  9392!).
VV     LYN    VB A (B 11.76M, 38.6",354G); SB; MU ALFA=-0.0285S,MU
DELTA=
              =-0.274".
VW     LYN    P1=590S, P2=260S  9393!.
S      LYR    P VAR. MAX=2416186+432.01D*E (J.D.2415700-
              20100); MAX=2420961+445.83D*E (J.D.2420900-
              26500); MAX=2426748+429.01D*E (J.D.2426500-
              30700); MAX=2432357+441.88D*E (J.D.2432000-
              34600); OCE/SINCE J.D.2442500-CM. TA./SEE
              TABLE.
U      LYR    VB A (B 13.0M, 9.4", 182G). P VAR. MAX=2418345+
              +459.22D*E (J.D.2418000-27000); OCE/SINCE J.D.
              2432000-CM. TA./SEE TABLE.
V      LYR    OH MAEP/MASER.
W      LYR    P VAR. MAX=2415578+198.39D*E (J.D.2413000-
              19000); MAX=2420322+194.99D*E (J.D.2419000-
              25500); MAX=2431326+198.97D*E (J.D.2427000-
              31500); MAX=2432494+195.11D*E (J.D.2431500-
              36500); OCE/SINCE J.D.2437500-CM. TA./SEE
              TABLE.
Y      LYR    DS=0.8.
Z      LYR    P VAR. MAX=2418150+285.07D*E (J.D.2417500-
              22200); MAX=2423600+291.37D*E (J.D.2422200-
              29500); MAX=2430000+284.00D*E (J.D.2429500-
              36800); OCE/SINCE J.D.2436800-CM. TA./SEE
              TABLE.
RR     LYR    MU ALFA=-0.11", MU DELTA=-0.19".  FE/H!=-1.14; DS=6. -
              EKT AKO EPEMEHHO AMT (PAKTECK
              O OHOO CEHOBEH EKTA); =40.8D. CME-
              EHE A MAX O 0.14P; BEHA B MAX MEH-
              ETC B PEEAX O 0.6M, BEHA B MIN-O 0.1M
               3418!. COACHO  7270!, B MEHEH AMT
              EKTA AKO HAAETC K-4 OA, B KOH-
              E KOTOPOO AA EKTA AKO MEHETC CKA-
              KOM HA 0.25 . MAHTHOE OE MEHETC C EPO-
              OM CA  9339!./BLAZHKO EFFECT OF VARIABLE
              AMPLITUDE (PRACTICALLY TO COMPLETE DISAPPEARANCE OF
              BLAZHKO EFFECT); =40.8D. VARIATIONS OF MAX LIGHT
              PHASE UP TO 0.14P; MAGNITUDE IN MAX VAR IN THE RANGE
              UP TO 0.6M, THAT IN MIN VAR IN THE RANGE UP TO 0.1M
               3418!.ACCORDING TO  7270!, A CYCLE-4 YR IS PRESENT
              IN BLAZHKO EFFECT AMPLITUDE CHANGES; AT THE END OF
              THE CYCLE THE BLAZHKO EFFECT PHASE CHANGES ABRUPTLY
              BY 0.25. MAGNETIC FIELD STRENGTH VARIES WITH THE
              PULSATIONAL PERIOD  9339!.
              P VAR. MAX=2414856.480+0.56682069D*E (J.D.
              2414800-18800); MAX=2421854.052+0.56685169D*E
              (J.D.2418800-26500)  9379!; MAX=2426571.3828+
              +0.56684333D*E (J.D.2426500-32500)  9338!; MAX=
              =2438215.9492+0.566830D*E (J.D.2438000-41000)
               5238!; MAX=2438215.9492+0.56683313D*E (J.D.
              2441000-42900)  9338!; OCE/SINCE J.D.2442900-
              CM. TA./SEE TABLE.
RS     LYR    P VAR. MAX=2415566+299.38D*E (J.D.2415000-
              24000); MAX=2425176+308.08D*E (J.D.2424000-
              37200); OCE/SINCE J.D.2437200-CM. TA./SEE
              TABLE.
RT     LYR    P VAR. MAX=2437022+250.85D*E (J.D.2415000-
              39000); OCE/SINCE J.D.2439000-CM. TA./SEE
              TABLE.
RU     LYR    P VAR. MAX=2415983+370.70D*E (J.D.2415900-
              33000); MAX=2433035+363.0D*E (J.D.2433000-
              41000); OCE/SINCE J.D.2441000-CM. TA./SEE
              TABLE.
RV     LYR    D=0.015P. P VAR. MIN=2415949.7096+3.599007D*E
              (J.D.2412185-16000); MIN=2415949.7096+
              +3.599046D*E (J.D.2416000-21400)  0001!; MIN=
              =2432015.671+3.5989845D*E (J.D.2421400-32000);
              MIN=2432015.671+3.5990235D*E (J.D.2432000-
              39300)  9085!; OCE/SINCE J.D.2442000-CM. TA./
              SEE TABLE.
RW     LYR    OH, H2O MAEP/MASER.
RX     LYR    P VAR. MAX=2416226+249.94D*E (J.D.2415000-
              28800); OCE/SINCE J.D.2428800-CM. TA./SEE
              TABLE.
RZ     LYR    P VAR. MAX=2416415.360+0.51127069D*E (J.D.
              2413000-19000)  0001!; MAX=2426161.4375+
              +0.51124948D*E (J.D.2426000-38000)  0323!; OCE/
              SINCE J.D.2438000-CM. TA./SEE TABLE.
              EKT AKO, MEHETC BCOTA MAX:/BLAZHKO
              EFFECT, HEIGHT OF MAX VARIES: 10.6M-10.9M, MAX (DM)=
              =2430904.3+116.654D*N+0.01034D*N**2; MIN (DM)-
              -MAX (DM)=59.3D  3419!.
               FE/H!=-1.69; DS=10.0.
SS     LYR    P VAR. MAX=2421695+350.48D*E (J.D.2416000-
              22500); MAX=2429991+355.22D*E (J.D.2429000-
              38000); OCE/SINCE J.D.2438000-CM. TA./SEE
              TABLE.
SZ     LYR    COACHO  5750!, B HTEPBAE J.D.2434665-35044
              AMTA A BBOE MEHE OHO (A CET
              H MIN)  ME MECTO BPEMEHH CO A
              HA 0.5P./ACCORDING TO  5750!, DURING J.D.2434665-
              35044 THE AMPLITUDE WAS TWICE SMALLER THAN USUAL
              (DUE TO THE DEPTH OF MIN), AND A TEMPORARY PHASE
              SHIFT BY 0.5P OCCURED.
TT     LYR    D=0.010P; MIN II 9.44.
TW     LYR    VB A (B 15.2M PG, 14".70G, 1912).
TY     LYR    P VAR. MAX=2419285+336.49D:*E (J.D.2419000-
              23700); MAX=2423985+329.79D*E (J.D.2423700-
              31250); OCE/SINCE J.D.2438600-CM. TA./SEE
              TABLE.
TZ     LYR    VB A (B 12.29M, 2.54", 2.5G). MIN II 11.05. P VAR.
              MIN I=2420669.480+0.5288234D*E (J.D.2420000-
              38000); OCE/SINCE J.D.2438000-CM. TA./SEE
              TABLE.
UX     LYR    B-V:+0.11, +0.47.
UZ     LYR    D=0.012P:. P VAR. MIN=2424268.474+1.891253D*E
              (J.D.2422500-25500)  2087!; OCE/SINCE J.D.
              2425500-CM. TA./SEE TABLE.
AA     LYR    MIN II 13.5.
AH     LYR    D=0.03P. MIN II 12.1.
AK     LYR    MIN II 12.9.
AL     LYR    P VAR. MAX=2427865.82+12.9837D*E (J.D.2414800-
              28000)  0001!; MAX=2432889.03+12.98047D*E (J.D.
              2428000-35500)  4427!; OCE/SINCE J.D.2435500-
              CM. TA./SEE TABLE.
AQ     LYR    P VAR. MAX=2425301.592+0.3571721D*E (J.D.2425300-
              29000); MAX=2428944.739+0.3571285D*E (J.D.
              2429000-30200); MAX=2430158.976+0.3571611D*E
              (J.D.2430200-33900); MAX=2433909.178+
              +0.3571861D*E (J.D.2433900-35700); B HTEPBAE/
              DURING J.D.2435700-37800-CM. TA./SEE TABLE.
              EKT AKO? O BAHM HAEHM/
              BLAZHKO EFFECT? ACCORDING TO VISUAL OBSERVATIONS,
              0.4M<=DM<=1.2M.
AY     LYR    K CBEPXMAKCMMOB/CYCLES OF SUPERMAXIMA
              188.9D-212.8D. EPOECKE KOEAH B CBEPX-
              MAKCMMAX:/SUPERHUMPS PERIOD: PS=0.07552D
               6249!.
BF     LYR    P VAR. MAX=2425296+130D*E (J.D.2425300-800);
              B HTEPBAE/DURING J.D.2429045-570-CM. TA./
              SEE TABLE.
BH     LYR    P VAR. MAX=2413712.358+0.6129028D*E (J.D.
              2413712-27927); MAX=2434472.547+0.6128941D*E
              (J.D.2434472-36102); OCE/SINCE J.D.2436423-
              CM. TA./SEE TABLE.
BQ     LYR    DS=0:.
BV     LYR    D=0.025P.
CC     LYR    P VAR. MAX=2433182.7+24.028D*E (J.D.2426100-
              33400); MAX=2437078.8+24.200D*E (J.D.2433400-
              37100)  0001!; MAX=2439418.5+24.185D*E (J.D.
              2437100-39420)  5644!; OCE/SINCE J.D.2440400-
              CM. TA./SEE TABLE.
              OPMA KPBO ECKA/LIGHT CURVE SHAPE VAR?
               A/H!=-2.2.
CV     LYR    BOMOHO HAOEHE/POSSIBLE SUPERPOSITION OF
              P2=135D.
CX     LYR    P VAR. MAX=2418596.111+0.616689D*E (J.D.
              2414880-20000); MAX=2427696.396+0.616669D*E
              (J.D.2427530-30610); OCE/SINCE J.D.2433000-
              CM. TA./SEE TABLE.DS=7:.
DD     LYR    P VAR. MAX=2425494.334+0.372610D*E (J.D.
              2418900-27600)  0001!; OCE/SINCE J.D.2427600-
              CM. TA./SEE TABLE.
DF     LYR    MIN II 13.4.
DI     LYR    P VAR. MAX=2437160.310+0.4174486D*E (J.D.
              2437160-39293); MAX=2439293.468+0.4178451D*E
              (J.D.2439293-40768); OCE/SINCE J.D.2440768-
              CM. TA./SEE TABLE.
DN     LYR    P2=600D.
DR     LYR     FE/H!=-1.41; DS=7.4.
DU     LYR    MIN II 13.3.
EN     LYR    B-V:+0.40.+0.43. P VAR. DM VAR.
EP     LYR    MAX I =0.20P; MIN II 10.36M-10.58M,  =0.50P; MAX II
              10.01M-10.10M,  =0.70P. BTOPHE KOEAH:/
              SECONDARY OSCILLATIONS: P2=45.1D,  P3=7067D  9354!.
EW     LYR    P VAR; KBAPATH EH:/NONLINEAR TERM:
              +0.00210D*10**-6*E**2 (J.D.2426500-45500);
              OCE J.D.2442000 HAEH PECTABTC
              TAKE EMEHTAM:/SINCE J.D.2442000 THE OBSER-
              VATIONS ARE REPRESENTED ALSO BY THE ELEMENTS: MIN=
              =2445597.391+1.948763D*E  7037, 0001!.
EX     LYR     FE/H!=-0.63; DS=2.5.
EZ     LYR    VB A (B 12.3M, 14", 302G, 1934). P VAR. OCE/SINCE
              J.D.2426577-CM. TA./SEE TABLE. DS=7.1.
FG     LYR    VB A (B 14M, <10"). D=0.035P. P VAR?
FH     LYR    P VAR?
FK     LYR    OTOECTBEHE C HDE 337663(G5)  0021! HEBEPHO./
              THE IDENTIFICATION WITH HDE 337663(G5)  0021! IS
              WRONG.
FL     LYR    MIN II 9.52,  DII=0.05P.
FN     LYR    B-V:+0.15, +0.48.
FO     LYR    MIN II 13.7.
GY     LYR    EMEHT OPEEEH  PAX MAKCMMOB.
              ME HM-2-3 BOH C MEHE AMTO.
              KPACHA./THE ELEMENTS DESCRIBE THE BRIGHTEST MA-
              XIMA. BETWEEN THEM IHERE ARE 2-3 WAVES OF SMALLER
              AMPLITUDE. RED.
HP     LYR    MIN II 11.0.
HQ     LYR    P VAR, EPOECK EH:/PERIODIC TERM:
              +30D SIN(8G*E).
HT     LYR    MIN II 13.3.
HY     LYR    MIN II 14.1.
IK     LYR    EKT AKO?/BLAZHKO EFFECT?
IL     LYR    COACHO/ACCORDING TO  0569!, MAX=2429375.519+
              +0.377620D*E, M-M=0.14P:.
IO     LYR    DS=3.
IP     LYR    MIN II 13.3.
IW     LYR    MIN II 13.3.
IY     LYR    MIN II 14.1.
KM     LYR    EKT AKO:/BLAZHKO EFFECT: =30D, 0.14P<=
              <=M-M<=0.20P.
KP     LYR    ADS 11423 C (A 8.5M, B 9.7M; AB-C 77", 208G; D 13.1M,
              C-D 14", 61G, 1904). P2=1300D BOMOEH/IS POS-
              SIBLE.
KR     LYR    P VAR. OPMA KPBO ECKA/THE LIGHT CURVE SHAPE
              VAR.
KT     LYR    MIN II 14.9.
KX     LYR    DS=0.
LQ     LYR     FE/H!=-1.39; DS=7.2.
LR     LYR    P VAR?  FE/H!=-1.41; DS=7.4.
LT     LYR    HAAC CTPE MEHEH (0.5M B AC)./RA-
              PID VARIATIONS (0.5M IN AN HOUR) WERE OBSERVED.
LX     LYR    DS=8:.
LZ     LYR    P VAR. MIN=2425347.565+1.611143D*E (J.D.2425347-
              32119)  0569!; OCE/SINCE J.D.2442870-CM. TA./
              SEE TABLE.
MN     LYR    MIN II 14.1.
MR     LYR    PO BOMOH P/ALTERNATIVE P=0.66D:.
MS     LYR    P<0.5D?
MT     LYR    MIN II 16.2.
MV     LYR    SB (PORB=0.1336D  9373!). KBAEPOECKE OC-
              AEH ECKA PAHO AMT:/QUASIPERIODIC
              FADINGS OF DIFFERENT AMPLITUDE: MIN=2425558+455.5D*E
              (J.D.2425500-30100); MIN=2430113+325.3D*E (J.D.
              2430100-36900); MIN=2436944+357.8D*E (J.D.
              2436900-44100)  9372!.
              OCE J.D.2444100 CPEH POBEH ECKA A
              HA 5M; HAATC BCK C AMTO O 3M
              POOTEHOCT 1-2 MEC.  9404!. P BCOKOM
              POBHE ECKA HAATC KTA O 0.4M A
              5 MH. B AX U  0365!. MK PEHTEHOBCK
              CTOHK./AFTER J.D.2444100 THE MEAN BRIGHTNESS
              LEVEL BECAME FAINTER BY 5M; OUTBURSTS WITH AN AMPLI-
              TUDE UP TO 3M OF 1-2 MONTHS DURATION ARE OBSERVED
               9404!. DURING THE BRIGHT LEVEL OF LIGHT, FLICKERING UP
              TO 0.4M IN 5 MIN IN U BAND IS OBSERVED  0365!. SOFT
              X-RAY SOURCE.
              B-V: 0.00+-0.40; U-: -0.86+-1.30.
MW     LYR    P VAR. MAX=2429521.386+0.3978817D*E (J.D.
              2427700-36000); OCE/SINCE J.D.2436000-CM.
              TA./SEE TABLE.
              EKT AKO:/BLAZHKO EFFECT: =33.3D; AM-
              TA MEHETC HA 0.6M/THE AMPLITUDE VARIES BY
              0.6M.
MZ     LYR    MIN II 14.0.
NV     LYR    D=0.02P:.
NW     LYR    P VAR. MAX=2436483.323+1.6012330D*E (J.D.2414500-
              36400)  3506!; OCE/SINCE J.D.2436400-CM. TA./
              SEE TABLE.
              B-V:+0.38, +0.86.
NY     LYR    MIN II 13.1.
NZ     LYR    O-C MEHTC CHCOAHO C AMTO +-0.01D./
              O-C VARY HARMONICALLY WITH AN AMPLITUDE +-0.01D,
              -2500P.
OQ     LYR    VB (B 12.1M VIS, 5.3", 175G, 1930).
OS     LYR    40D<=P<=60D. P2=400D-500D HAKABAETC/IS SU-
              PERIMPOSED.
PQ     LYR    D=0.014P; MIN II 14.9.
PS     LYR    D=0.02P:; MIN II 11.4.
PU     LYR    KE CTHK/CLOSE COMPANIONS SF, S.
PV     LYR    D=0.03P:.
PY     LYR    MIN II 13.4. P VAR. MIN I=2434980.4372+0.38576671D*E
              (J.D.2432700-36900)  4248!; OCE/SINCE J.D.
              2442500-CM. TA./SEE TABLE.
QQ     LYR    MIN II 14.6.
QT     LYR    MIN II 14.6.
QU     LYR    MIN II 13.1.
V335   LYR    CHOE PACCEHE HA KPBO ECKA./LARGE SCAT-
              TER IN THE LIGHT CURVE.
V336   LYR    P VAR. MIN=2429965.283+1.9049105D*E (J.D.
              2429370-31590); B HTEPBAE/DURING J.D.2438930-
              40010-CM. TA./SEE TABLE.
V337   LYR    CM./SEE V335 LYR.
V348   LYR    MIN II 16.8. EMEHT CPABEB B HTEPBAE/
              THE ELEMENTS ARE VALID DURING J.D.2444023-45232.
V350   LYR    P VAR. EMEHT ECTBT B HTEPBAE/THE ELE-
              MENTS ARE VALID DURING J.D.2438280-45232.
V355   LYR    EMEHT CPABEB B HTEPBAE/THE ELEMENTS
              ARE VALID DURING J.D.2429322-45232.
V356   LYR    VB A (B 17.5M, 10", 120G  0001!).
V361   LYR    MIN II 15.3, MAX II 14.7, MAX II-MIN I=0.70P. EMEH-
              T ECTBT B HTEPBAE/THE ELEMENTS ARE VALID
              DURING J.D.2433776-45232).
V374   LYR    CAE CTHK/FAINT COMPANIONS NP, SF.
V380   LYR    K CA CTHK/FAINT CLOSE COMPANION NF.
V385   LYR    K CA CTHK/FAINT CLOSE COMPANION SF.
V388   LYR    HE HAAOC OPAH B HTEPBAE/NO BRIGHTE-
              NINGS WERE OBSERVED DURING J.D.2438322-39289.
V389   LYR    EMEHT ECTBT B HTEPBAE/THE ELEMENTS
              ARE VALID DURING J.D.2438322-40007.
V390   LYR    EMEHT ECTBT B HTEPBAE/THE ELEMENTS
              ARE VALID DURING J.D.2439913-40007.
V401   LYR    MIN II 14.4:. EPO, BOMOHO, KAC./THE
              PERIOD MAY BE SPURIOUS.
V403   LYR    P VAR?, =500 P?
V404   LYR    MIN II 12.4.
V406   LYR    MIN II 13.0.
V409   LYR    P VAR? EMEHT ECTBT B HTEPBAE/THE ELE-
              MENTS ARE VALID DURING J.D.2434500-40000.
              EKT AKO?/BLAZHKO EFFECT?
V411   LYR    MIN II 14.4. BOMOHO, RRC/ALTERNATIVELY RRC (P=
              =0.291315D).
V412   LYR    MIN II 14.1; MIN II-MIN I=0.48P.
V413   LYR    MIN II 14.8?
V415   LYR    K/CYCLE<=150D.
V417   LYR    MIN II 16.2. P VAR?
V418   LYR    P VAR. EMEHT ECTBT B HTEPBAE/THE ELE-
              MENTS ARE VALID DURING J.D.2437100-40400.
V423   LYR    MIN II 15.5. P VAR?
V424   LYR    CM./SEE IK LYR.
V428   LYR    MIN II 14.3. BEHE H AC?/APSIDAL MO-
              TION?
V429   LYR    MIN II 14.8?
V431   LYR    MIN II 15.1.
V435   LYR    BOMOHO, EW C BOHM P. P MOET T KA-
              MC./POSSIBLY EW WITH TWICE LONGER P. P MAY
              BE SPURIOUS.
V462   LYR    P VAR? EMEHT ECTBT B HTEPBAE/THE
              ELEMENTS ARE VALID DURING J.D.2439913-40007.
V467   LYR    MIN II 12.9. EMEHT CPABEB B HTEPBAE
              J.D.2415288-43287; OO PAPOC HA KPBO
              ECKA. COACHO  9412!, B HTEPBAE J.D.
              2443424-44165 PEE MEHEH ECKA 12.4M-
              12.6M PG, EMEHT HE ECTBT./THE ELEMENTS
              ARE VALID DURING J.D.2415288-43287; LARGE SCATTER
              ON THE LIGHT CURVE. ACCORDING TO  9412!, DURING J.D.
              2443424-44165 THE LIGHT VARIATION RANGE IS 12.4M-
              12.6M PG, THE ELEMENTS ARE NOT VALID.
V470   LYR    U=0.40", P=7G. P1=738.6S, P2=557.4S, P3=318.0S,
              P4=291.9S, P5=259.1S.
V473   LYR    P VAR, DM VAR. COACHO/ACCORDING TO  9413!, P=
              =1.490795D+1.22D*10**-6*(J.D.-2443600)/365.25D.
              K B MEHEH P:/CYCLIC P VARIATIONS: PALFA=
              =1178.5D; PT=2655D.
              DM MEHETC C EPOOM PALFA; B MEHEHX VR
              POCEBAETC P4=1063.5D./DM VARIES WITH THE PE-
              RIOD PALFA; P4=1063.5D MAY BE TRACED IN THE VARIATIONS
              OF VR.
              0.06M<=DM<=0.36M.
V474   LYR    P2=76D.
V477   LYR    EHTPAHA BEA AHETAPHO TMAHHOCT
              ABELL 46. CH EKT OTPAEH./THE CENTRAL
              STAR OF PLANETARY NEBULA ABELL 46. STRONG REFLEC-
              TION EFFECT.
              H MHMMOB:/DEPTHS OF MINIMA: MIN I 1M. 42B,
              MIN II-0M. 1B.
ALFA   LYR    K TOK/IR EXCESS.
BETA   LYR    ADS 11745 A (B 8.6M, B7V, 46", 149G; C 13.0M, 47",
              248G). MIN II 3.85. P VAR.
              HEHEHE EH:/NONLINEAR TERMS:+3.883D*10**-6*
              *E**2-0.10D*10**-10*E**3.
              OPMA KPBO ECKA VAR. PAO-  PEHTEHOB-
              CK CTOHK. K TOK./LIGHT CURVE SHAPE VAR.
              RADIO- AND X-RAY SOURCE. IR EXCESS.
DELTA* *2     LYR EH PACCEHHOO CKOEH/OPEN CLUSTER DELTA**2 LYR
              MEMBER  2505!.
R      MEN    HOA/SOMETIMES P=120D;
              HOA/SOMETIMES P=240D.
T      MEN    CM./SEE RS MEN. EMEHT COEPAT KBAPAT-
              H EH:/THERE IS A SGUARE TERM IN THE ELEMENTS:
              +8.1D*10**-6*E**2.
U      MEN    VB A (B 10.4M, 0.6", 71G, 1935.3). A VAR (0.8M<=A<=2.9M).
              P VAR. MAX=2416927+426.9D*E (J.D.2415200-17400)
               0207!; OCE/SINCE J.D.2417400-CM. TA./SEE
              TABLE.
V      MEN    OXA COOTBETCTBET CEPEHE BOCXOE BETB
              KPBO ECKA./EPOCH CORRESPONDS TO THE MIDDLE OF
              THE LIGHT CURVE ASCENDING BRANCH.
W      MEN    EH OOO MAEAHOBA OAKA./THE MEMBER
              OF THE LARGE MAGELLANIC CLOUD.
RR     MEN    MIN II 12.1.
RS     MEN    B OACT OOO MAEAHOBA OAKA; HE EH
              OAKA/IN THE LARGE MAGELLANIC CLOUD REGION; NOT
              A MEMBER OF THE CLOUD.
RT     MEN    CM./SEE RS MEN.
RU     MEN    CM./SEE RS MEN.
RV     MEN    CM./SEE RS MEN.
RW     MEN    CM./SEE RS MEN.
TU     MEN    PORB=0.1176D  9376!. EPO CBEPXOPOB/SUPERHUMP
              PERIOD PS=0.12625D  4772!.
TY     MEN    MIN II 8.47; D I=0.00P, D II=0.07P. OPMA KPBO
              ECKA MEHETC/SHAPE OF THE LIGHT CURVE VARIES.
TZ     MEN    MIN II 6.36.
UX     MEN    MIN II 9.47; MIN II-MIN I=0.50045P. OH  KOM-
              OHEHTOB MOET T ECKO EPEMEHHO./ONE
              OF THE COMPONENTS MAY BE A PHYSICAL VARIABLE.
WY     MEN    B PAOHE APOBOO CKOEH NGC 1841; HE EH
              CKOEH. B AO CCTEM MAEAHOBX OA-
              KOB./IN THE REGION OF THE NGC 1841 GLOBULAR CLUS-
              TER; NOT A MEMBER OF THE CLUSTER. IN THE HALO OF THE
              MAGELLANIC CLOUDS SYSTEM.
WZ     MEN    CM./SEE WY MEN.
XX     MEN    CM./SEE WY MEN.
XY     MEN    CM./SEE RS MEN. MIN II 10.88; DI=0.05P; DII=0.00P.
XZ     MEN    OHOBPEMEHHO HAATC TP KOEAH:/THERE
              ARE THERE OSCILLATIONS SIMULTANEOUSLY: P1=0.1083D
              (A1=0.0094M B), P2=0.0855D (A2=0.0082M B), P3=
              =0.0955D (A3=0.0058M B); P2/P1=0.789.
IOTA   MEN    MIN II 6.05.
R      MIC    P VAR. MAX=2413373+138.60D*E (J.D.2413300-
              29600)  0458!; MAX=2432745+137.43D*E (J.D.
              2429600-34700); MAX=2435091+140.84D*E (J.D.
              2434700-37800); OCE/SINCE J.D.2437800-CM.
              TABL./SEE TABLE.
S      MIC    P VAR. MAX=2413499+214.5D*E (J.D.2413500-
              15900)  0458!; MAX=2432102+208.23D*E (J.D.
              2422700-32200); OCE/SINCE J.D.2432200-CM.
              TABL./SEE TABLE.
U      MIC    OH, H2O MCC/EMISSION.
V      MIC    CM./SEE U MIC.
Y      MIC    CPEH ECK MEHETC./MEAN BRIGHTNESS VARIES.
Z      MIC    (K-B)2=0.12; DS=4.
RR     MIC     A/H!=-1.4. P VAR. MAX=2433032.96+31.78175D*E
              (J.D.2415000-35300)  2747!; OCE/SINCE J.D.
              2443600-CM. TA./SEE TABLE.
RY     MIC    P VAR? PBEEHHE B TAE EMEHT PECTAB-
              T HAEH B HTEPBAE/ELEMENTS GIVEN IN
              THE TABLE REPRESENT OBSERVATIONS IN THE INTERVAL J.D.
              2436100-40210.
              COACHO/ACCORDING TO  0085! MAX=2428670+
              +190D*E.
RZ     MIC    MIN II 11.2.
TV     MIC    MIN II 12.4.
UZ     MIC    MIN II 12.4.
VW     MIC    B HTEPBAE/IN THE INTERVAL J.D.2436600-840)
              MAX=2436807.248+0.35620D*E. OCE/SINCE J.D.
              2442600-CM. TA./SEE TABLE.
WY     MIC    P=0.511427D?  0001!.
XZ     MIC    B HTEPBAE/IN THE INTERVAL J.D.2436670-840 MAX=
              =2436731.480+0.449208D*E. OCE/SINCE J.D.
              2442630-CM. TA./SEE TABLE.
ZZ     MIC    (K-B)2=021; DS=0. P VAR? MAX=2437192.3131+
              +0.0671786D*E (J.D.2437180-460)  4308!; MAX=
              =2439320.2162+0.0671575D*E (J.D.2439320-340)
               5683!; OCE/SINCE J.D.2440440-CM. TA./SEE
              TABLE.
              BOMOHO AHEEE BEEHE EPOA  9380!.
              COACHO  7985! OHOBPEMEHHO HAATC BA
              KOEAH C EPOAM P1  P2:/FURTHER PERIOD
              INCREASE IS POSSIBLE  9380!. ACCORDING TO  7985!
              THERE ARE TWO SIMULTANEOUS OSCILLATIONS WITH THE
              PERIODS P1 AND P2: P1=0.0654D, P2=0.0513D.
              P2/P1=0.784; A2(U)=0.25 A1(U).
AE     MIC    B HTEPBAE/IN THE INTERVAL J.D.2436670-840 MAX=
              =2436728.470+0.324142D*E. OCE/SINCE J.D.
              2442630-CM. TA./SEE TABLE.
AH     MIC    MIN II 13.6.
AT     MIC    VB (A 10.83M V, M 4.5VE; B 10.9M V, M 4.5VE; A=
              =6.40", P=675 YR, E=0.60  9381!. MU ALFA=+0.0216S,MU
DELTA=
              =-0.331" (MU, VR, PI-OE C/COMMON WITH AU MIC).
              HEOHO OA ACTOTA BCEK OBOET
              CTAT,  TO MEHTC OA KOMOHEHTA. B TA-
              E PBEEH PEE MEHEH CMMAPHOO
              ECKA CCTEM./UNUSUALLY HIGH FREGUENCY OF FLARES
              ALLOWS TO SUPPOSE THAT BOTH COMPONENTS ARE VARIABLE.
              THE RANGE OF COMBINED BRIGHTNESS VARIATION OF THE
              SYSTEM IS GIVEN IN THE TABLE.
AU     MIC    MU ALFA=+0.0212S, MU DELTA=-0.348" (MU, PI, VR-OE
C/COM-
              MON WITH AT MIC).
              SB? 0.20P<=M-M<=0.55P. HAP C EPOECKM
              MEHEHM ECKA HAATC BCK C
              A<=0.5M U/THERE ARE PERIODICAL LIGHT VARIATIONS AND
              ALSO FLARES WITH A<=0.5M U  8601!.
AW     MIC    MU ALFA=+0.0077S, MU DELTA=-0.089". OPMA KPBO ECKA
              CHO MEHETC. BOMOHA MTEPOHOCT./
              SHAPE OF THE LIGHT CURVE STRONGLY VARIES. MULTIPERIO-
              DICITY IS POSSIBLE.
AX     MIC    MU ALFA=-0.2805S, MU DELTA=-1.152". B MHMME ECKA/IN
              MINIMUM BRIGHTNESS B-V=+1.42, U-B=+1.20.
R      MON    EKPH HEBEH O'EKT, PACOOEHH B
              BEPHE OTPAATEHO EPEMEHHO  9396! KOME-
              TOOPAHO TMAHHOCT NGC 2261. O-BMOM,
              MOOA BEA, OKPEHHA EBM OAKOM.
              PAK KPBO ECKA  9394!./PECULIAR NON-STEL-
              LAR OBJECT AT THE APEX OF THE REFLECTION VARIABLE  9396!
              COMETARY NEBULA NGC 2261. PROBABLY YOUNG STAR SUR-
              ROUNDED BY DUST CLOUD. LIGHT CURVE IN  9394!.
S      MON    B PACCEHHOM CKOEH/IN THE OPEN STAR CLUSTER
              NGC 2264. VB A (B 8.2M, 2.9", 213G; 9.9M, 16.6", 14G).
T      MON    SB (PORB>=70 YR  9397!).  A/H!=0.3. PBEEHHE B
              TAE EMEHT COEPAT KBAPATH EH:/
              THERE IS A SGUARE TERM IN THE ELEMENTS GIVEN IN THE
              TABLE:+5.34D*10**-6*E2.
              OTKOHEH OT APAO HA APAMME O-C, E
              MET BOHOOPAH XAPAKTEP. EC OH O'CH-
              TC OPTAHM BEHEM, TO PORB=100 ET./
              DEVIATIONS FROM THE PARABOLA IN THE O-C, E DIAGRAM
              HAVE A WAVE-LIKE TREND. IF THIS WAVE IS ATTRIBUTED TO
              THE LIGHT-TIME EFFECT, PORB=100 YEARS.
              HAEH MOHO PECTABT TAKE CEE
              CCTEMO HEHX EMEHTOB:/THE OBSERVATIONS
              ARE ALSO SATISFIED BY THE FOLLOWING SYSTEM OF LINEAR
              ELEMENTS: MAX=2412874.56+27.0093D*E (J.D.
              2405200-15250)  9398!; MAX=2426004.62+27.0180D*E
              (J.D.2415250-27150); OCE/SINCE J.D.2427150-
              MAX=2436137.090+27.0205D*E  2392!.
U      MON    P VAR. MIN=2408897+92.26D*E (J.D.2408800-
              36210)  0368!; OCE/SINCE J.D.2437300-CM. TA./
              SEE TABLE.
              CPEH BEHA MEHETC C EPOOM 2320D
               0657!. CCEOBAHE CEKTPA  2226!./MEAN MAG-
              NITUDE VARIES WITH THE PERIOD 2320D  0657!. SPECTRUM
              INVESTIGATION  2226!.
V      MON    P VAR. MAX=2412172+334.5D*E (J.D.2412000-
              23500)  0458!; MAX=2427870+332.5D*E (J.D.2423500-
              28200); MAX=2429904+342.0D*E (J.D.2428200-
              30800); MAX=2439570+331.6D*E (J.D.2430800-
              41225); OCE/SINCE J.D.2441225-CM. TA./SEE
              TABLE.
X      MON    P VAR. MAX=2415078+154.0D*E (J.D.2415000-
              18800); MAX=2419758+149.6D*E (J.D.2419700-
              21000); MAX=2421136+155.0D*E (J.D.2421000-
              24600); MAX=2424673+169D*E (J.D.2424600-
              25600); MAX=2425644+155.6D*E (J.D.2425600-
              26800); MAX=2427028+150.7D*E (J.D.2427000-
              28000)  0458!; MAX=2429521+155.8D*E (J.D.
              2428000-36300); MAX=2438846+145.3D*E (J.D.
              2437800-38900); OCE/SINCE J.D.2440800-CM.
              TA./SEE TABLE.
              AMTA CHO MEHETC; HOA HAATC
              HEPABHE MEHEH ECKA./THE AMPLITUDE
              STRONGLY VARIES; SOMETIMES IRREGULAR LIGHT VARIATIONS
              ARE OBSERVED.
Y      MON    P VAR. MAX=2415792+228.6D*E (J.D.2415300-
              19700); MAX=2419928+227.4D*E (J.D.2419700-
              24300)  0458!; MAX=2432647+233.3D*E (J.D.
              2424300-32900); OCE/SINCE J.D.2432900-CM.
              TA./SEE TABLE.
RR     MON    P VAR. MAX=2417476+384.5D*E (J.D.2417400-
              19600)  0458!; OCE/SINCE J.D.2419600-CM. TA./
              SEE TABLE.
RU     MON    MIN II 11.06; D II VAR: 0.06P<=DII<=0.12P; MIN II-MIN I
              VAR: 0.25P<=MIN II-MIN I<=0.75P. P VAR. B HTEPBAE/
              IN THE INTERVAL J.D.2429100-38409 MIN I=
              =2418357.0140;3.5846794D(E-406)-0.429D COS ALFA+
              +0.06D SIN 2ALFA+0.010D COS 3ALFA+0.003D SIN 4ALFA, MIN
II=
              =2418355.2220+3.5846794D(E-406)+0.429D COS ALFA+
              +0.060D SIN 2ALFA-0.010D COS 3ALFA+0.003D SIN 4ALFA (J.D.
              2416900-29100); MIN I=2429641.567+3.5846391D*
              (E-3554)-0.429D COS ALFA+0.060D SIN 2ALFA+0.010D*
              *COS 3ALFA+0.003D SIN 4ALFA, MIN II=2429639.775+
              +3.5846391D(E-3554)+0.429D COS ALFA+0.060D SIN 2ALFA-
              -0.010D COS 3ALFA+0.003D SIN 4ALFA, E/WHERE ALFA=
              =0.01245G(E-406)  3445!.
              CET OX E BEETC  MIN I OT J.D.HEL.
              2416901.205, A  MIN II-OT J.D.HEL.
              2416900.248/THE EPOCHS E ARE BEING CALCULATED FOR
              MIN I FROM J.D. HEL. 2416901.205, AND FOR MIN II-
              FROM J.D. HEL. 2416900.248.
              B HTEPBAE/IN THE INTERVAL J.D.2438409-41743
              MIN I=2438409.6045+3.584586D(E-6000)-0.4290D*
              *COS ALFA+0.0620D SIN 2ALFA+0.0107D COS 3ALFA+0.0026D*
              *SIN 4ALFA-0.00036D COS 5ALFA, MIN II=2438407.8122+
              +3.584586D(E-6000)+0.4290D COS ALFA+0.0620D SIN 2ALFA-
              -0.0107D COS 3ALFA+0.0026D SIN 4ALFA+0.00036D COS 5ALFA,
              E/WHERE ALFA=0.012385G(E-406)  7987!.
              OCE/SINCE J.D.2441743-MIN I=2441743.2633+
              +3.584670D(E-6930)-0.4336D COS ALFA+0.0634D SIN 2ALFA+
              +0.0111D COS 3ALFA+0.0021D SIN 4ALFA, MIN II=
              =2441741.4710+3.584689D(E-6930)+0.4336D COS ALFA+
              +0.0634D SIN 2ALFA-0.0111D COS 3ALFA+0.0021D SIN 4ALFA,   /
E
              WHERE ALFA=70.6G+0.0114G(E-6094)  9546!.
              B TAE PBEEH HEHE EMEHT, KOTOPE
              OH PECTABT OX MIN I B 1973-1990 .
              COOTBETCTBE EMEHT  OX MIN II ME-
              T B:/LINEAR ELEMENTS FOR MIN I EPOCHS IN 1973-
              1990 ARE GIVEN IN THE TABLE. CORRESPONDING ELEMENTS
              FOR MIN II EPOCHS ARE: MIN II=2441741.575+
              +3.584567D*E. E=0.38. EPO BPAEH H A-
              C-285 ET./APSIDAL MOTION PERIOD IS 285 YEARS.
RV     MON    CPEH BEHA MEHETC C P=1047D./MEAN
              BRIGHTNESS VARIES WITH P=1047D.
RW     MON    MIN II 9.45; D I=0.027P, D II=0.023P. P VAR. MIN I=
              =2417943.687+1.9061012D*E (J.D.2417940-32900)
               3450!; OCE/SINCE J.D.2432900-CM. TA./SEE
              TABLE.
RX     MON    P VAR. MAX=2418980+343.2D*E (J.D.2416200-
              19000); MAX=2423097+338.9D*E (J.D.2422000-
              28500); OCE/SINCE J.D.2428500-CM. TA./SEE
              TABLE.
RY     MON    VB A (B 12.29M, 28").
SS     MON    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 2264.
SU     MON    S 5/7-S 6/7. P VAR: 69D (J.D.2416700-19100); 203.5D
              (J.D.2420100-22920); 69D (J.D.2423000-30100). B
              HTEPBAAX/IN THE INTERVALS J.D.2423000-520-
              CONST (11.5M), J.D.2424820-980-CONST (11.8M).
SV     MON     A/H!=0.2. P VAR. MAX=2419041.805+15.230721D*E
              (J.D.2412000-22000)  0025!; MAX=2422651.931+
              +15.23256D*E (J.D.2422600-23850)  9400!; MAX=
              =2424571.60+15.2513D*E (J.D.2423850-24600);
              MAX=2434045.326+15.2304D*E (J.D.2424600-34100);
              OCE/SINCE J.D.2433000-CM. TA./SEE TABLE.
SX     MON    CPEH ECK MEHETC C P=1100D/MEAN BRIGHT-
              NESS VARIES WITH P=1100D.
SZ     MON    VB A (B 11M-12M, 10"  9401!). MIN II 10.55. P VAR.
              MIN I=2426357.1+32.760D*E (J.D.2422000-26400);
              MIN I=2427861.2+32.708D*E (J.D.2426750-32000);
              OCE/SINCE J.D.2432800-CM. TA./SEE TABLE.
              OPMA KPBO ECKA MEHETC. BCOT MAKCM-
              MOB  H MHMMOB OCTOHH/SHAPE OF THE
              LIGHT CURVE VARIES. HEIGHTS OF MAXIMA AND DEPTHS OF
              MINIMA ARE CONSTANT.
TU     MON    MIN II 9.1.
TV     MON    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN STAR CLUSTER NGC 2237.
TW     MON    BAXMAH  3453! OTHOCT EPEMEHH K T RRAB C
              EMEHTAM MAX=2433001.371+0.8743887*E, HO
              OTMEAET HATEHOE PACCEHE TOEK BOKP
              CPEHE KPBO ECKA, OCTPOEHHO C TM EPO-
              OM. OCKOK EPO ECCHEP  BAXMAHA B-
              TC COPEHHM, B C OTMEEHHOO OCTO-
              TECTBA OEE BEPOTHO OTHOCTC K EEAM./
              WACHMANN  3453! ASSIGNS THE VARIABLE TO THE RRAB
              TYPE WITH THE ELEMENTS MAX=2433001.371+
              +0.8743887*E, BUT NOTES A CONSIDERABLE DISPERSION
              OF THE POINTS AROUND THE MEAN LIGHT CURVE OBTAINED
              WITH THIS PERIOD. AS THE PERIODS BY HESSNER (PH)
              AND WACHMANN (PW) ARE MUTUALLY RELATED (1/PW=
              =1/PH+1) IT IS MORE PROBABLE ON ACCOUNT OF THE
              ABOVE MENTIONED CIRCUMSTANCE THAT THE VARIABLE BE-
              LONGS TO CEPHEIDS.
TX     MON     A/H!=-0.3.
UV     MON    HEOHA  EPEMEHHX TA RR LYR OPMA
              KPBO ECKA (MAX II 13.5 HA AE 0.39P, MIN II 13.8
              HA AE 0.22P) ACTABET COMHEBATC B PAB-
              HOCT HAEH EPOA, HEABCMO HAEHHOO
              BM CCEOBATEM  0380, 3453!./THE FORM OF
              THE LIGHT CURVE BEING UNUSUAL FOR RR LYR TYPE VA-
              RIABLES (MAX II 13.5 AT THE PHASE 0.39P, MIN II 13.8
              AT THE PHASE 0.22P), THE PERIOD MAY BE DOUBTFUL,
              THOUGH IT WAS FOUND INDEPENDENTLY BY TWO INVESTIGA-
              TORS  0380, 3453!.
UX     MON    MIN II 8.52; DI=0.044P. P VAR? ECK B MAKCMME
              MEHETC B AMTO O 0.2M./BRIGHTNESS IN MA-
              XIMUM VARIES WITH THE AMPLITUDE UP TO 0.2M.
VV     MON    MIN II 9.55; DI=DII=0.07P. EMEHT, PBEEHHE
              B TAE, COEPAT KBAPATH EH:/THERE IS
              A SGUARE TERM IN THE ELEMENTS GIVEN IN THE TABLE:
              -0.12D*10**-7*E**2.
VW     MON    P VAR. MAX=2425243.40+0.6041350D*E (J.D.2414700-
              30700); OCE/SINCE J.D.2430700-CM. TA./SEE
              TABLE.
              B  0386, 5448!  PX PEHX PAOTAX PHMA-
              ETC COPEHHOE HAEHE EPOA 1.532D, PBO-
              EE K AKEH O HEOHOCT TO EPEMEH-
              HO. HH CEPEHE HAEH  BOPA C-
              THHOO HAEH./IN  0386, 5448! AND OFTER PRE-
              VIOUS WORKS THE SPURIOUS PERIOD VALUE 1.532D IS
              BEING ACCEPTED SUGGESTING THE CURIOUS NATURE OF THE
              VARIABLE. SERIOUS OBSERVATIONS ARE NECESSARY TO SE-
              LECT THE TRUE VALUE OF THE PERIOD.
VX     MON    HA MIN II/DEPTH OF MIN II 0.07M.
VY     MON    B PAOHE TMMAHHOCT/IN THE REGION OF THE NEBULA
              IC 446.
XX     MON     A/H!=-0.2.
XZ     MON    MIN II 13.6; D=0.02P:.
AA     MON     A/H!=-0.9. P VAR. MAX=2430788.266+3.938052D*E
              (J.D.2425300-34800)  3453!; OCE/SINCE J.D.
              2434800-CM. TA./SEE TABLE.
AC     MON    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 2323.
AK     MON    P VAR. MAX=2425279+319.2D*E (J.D.2425200-
              28000); OCE/SINCE J.D.2428000-CM. TA./SEE
              TABLE.
AN     MON    MIN II 11.7:; D=0.027P.
AO     MON    MIN II 10.16; DII=0.14P; MIN II-MIN I=0.4933P. P VAR.
              MIN I=2426735.333+1.884758D*E (J.D.2426700-
              40000); OCE/SINCE J.D.2440000-CM. TA./SEE
              TABLE.
AQ     MON    MIN II 10.9; DII=0.05P; DI=0.014P.
AR     MON    MIN II 9.03; D=0.011P. EMEHT, PBEEHHE B
              TAE, COEPAT KBAPATH EH:/THERE IS
              A SGUARE TERM IN THE ELEMENTS GIVEN IN THE TABLE:
              -1.22D*10**-6*E**2.
AU     MON    MIN II 8.2:. OPMA KPBO ECKA MEHETC./SHAPE
              OF THE LIGHT CURVE VARIES.
              ECK B MAKCMME MEHETC EPOECK C AM-
              TO 0.2M:/BRIGHTNESS IN MAXIMUM VARIES PERIO-
              DICALLY WITH THE AMPLITUDE 0.2M: MAX=2443105+
              +411D*E; M-M=0.5P.
AV     MON    HA MIN II/DEPTH OF MIN II 0.04M.
AW     MON    P VAR. MIN=2425649.053+20.797D*E (J.D.2425500-
              26400)  9408!; MIN=2426439.340+20.81905D*E (J.D.
              2426400-35900)  0511!; OCE/SINCE J.D.2435900-
              CM. TA./SEE TABLE.
AX     MON    BOHA CCTEMA C OOOKO  AOBM OTOKA-
              M. PORB=232.60D  6103!. CCEOBAHE CEKTPA
               9411!. B TAE PBEEHA OXA MIN ECKA,
              PEECTBA MOMEHT COEHEH HA 0.25P; A=
              =0.4M U. KPOME EPOECKX MEHEH, HA-
              ATC CTPE KTA ECKA O 0.1M./BINA-
              RY SYSTEM WITH AN ENVELOPE AND GASEOUS STREAMS.
              PORB=232.60D  6103!. SPECTRUM INVESTIGATION  9411!.
              EPOCH OF MIN BRIGHTNESS PRECEEDING THE MOMENT OF
              CONJUNCTION FOR 0.25P IS GIVEN IN THE TABLE; A=0.4M U.
              BESIDES PERIODICAL VARIATIONS, THERE ARE RAPID LIGHT
              FLUCTUATIONS UP TO 0.1M.
BB     MON    CM./SEE AV MON.
BC     MON    P VAR. MAX=2421240+275.8D*E (J.D.2421200-
              25960); MAX=2428880+267.2D*E (J.D.2425960-
              30000); OCE/SINCE J.D.2430000-CM. TA./SEE
              TABLE.
BE     MON    DS=0.
BH     MON    D=0.01P:.
BM     MON    MIN II 12.3. COACHO  9415!, BOMOHO BPAEHE
              H AC/ACCORDING TO  9415!, APSIDAL MOTION IS
              POSSIBLE.
BO     MON    MIN II 10.1. P VAR. MIN I=2428211.596+2.2251753D*E
              (J.D.2415000-36000)  0007!; OCE/SINCE J.D.
              2436000-CM.TA./SEE TABLE.
BP     MON    P VAR? PBEEHHE B TAE EMEHT OBET-
              BOPT HAEHM B HTEPBAE/ELEMENTS GIVEN
              IN THE TABLE ARE VALID IN THE INTERVAL J.D.2425600-
              29700.
BT     MON    VB A (B 16.0M, 10", 0G). OCE BCK B 1939 .
              ECK MEHETC B PEEAX 16.0M-18.7M C EMEH-
              TAM:/AFTER THE OUTBURST IN 1939 THE BRIGHTNESS VA-
              RIES IN THE RANGE 16.0M-18.7M WITH THE ELEMENTS: MIN=
              =2443491.7155+0.3338141D*E; D=0.20P, 0<=D<=0.03P.
              O BCK B 1939 ., COACHO  9417!, HAE-
              H OBETBOPC EMEHTAM:/BEFORE THE OUT-
              BURST IN 1939, ACCORDING TO  9417!, THE FOLLOWING ELE-
              MENTS WERE VALID: MIN=2429500.207+0.3338010D*E.
              B 1981 . BOKP HOBO OHAPEHA MCCOHHA
              TMAHHOCT PACOM 3.8"/EMISSION NEBULA WITH
              THE RADIUS OF 3.8" WAS DISCOVERED IN 1981 AROUND
              THE NOVA  9148!.
BX     MON    OHO OTHOCAC K EPEMEHHM TA MP KTA
               9421!. B TAE AHA OXA MAX ECKA  EP-
              O COACHO  9419!. COACHO  9420!, AMEPOB-
              CKE MCCOHHE H BOHKAT B TMAHHOCT,
              OKPAE CMOTECK CCTEM,  BO-
              ATC OPM KOMOHEHTOM, A MEHEH ECKA
              CBAH C OPTAHM BEHEM B TO CCTE-
              ME./USUALLY WAS CONSIDERED AS MIRA TYPE VARIABLE
               9421!. IN THE TABLE THE EPOCH OF LIGHT MAXIMUM AND
              THE PERIOD ARE GIVEN ACCORDING TO  9419!. ACCORDING
              TO  9420! THE BALMER EMISSION LINES ORIGINATE IN THE
              NEBULOSITY SURROUNDING THE SYMBIOTIC SYSTEM AND ARE
              EXCITED BY THE HOT COMPONENT, AND LIGHT VARIATIONS
              ARE DUE TO THE ORBITAL MOTION IN THE SYSTEM.
BZ     MON    D=0.030P. B PAOHE PACCEHHOO CKOEH/IN THE
              REGION OF THE OPEN CLUSTER CR 106.
CC     MON    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER CR 106.
CD     MON    P VAR. MAX=2427704+273.8D*E (J.D.2427400-
              30400); OCE/SINCE J.D.2430400-CM. TA./SEE
              TABLE.
CE     MON    MIN II 14.2.
CF     MON    MIN II 13.7; D=0.02P:.
CH     MON    D=0.030P.
CS     MON    VB A (B 13M, 9", 0G).
CT     MON    B PAOHE PACCEHHOO CKOEH/IN THE REGION
              OF THE OPEN CLUSTER NGC 2244.
CU     MON     A/H!=-0.2.
CV     MON    B EHTPE EMHHOO PACCEHHOO CKOEH./IN
              THE CENTRE OF AN ANONYMOUS OPEN CLUSTER.
              VB A (B 13.76M, 10", 270G; C 13.72M, 14", 270G).
              P VAR. MAX=2429805.142+5.378782D*E (J.D.2429360-
              36000); OCE/SINCE J.D.2436000-CM. TA./SEE
              TABLE.
DD     MON    MIN II 11.3.
DF     MON    KAPTA B  5285! HEBEPHA, HAAAC HE DF MON./
              THE CHART IN  5285! IS WRONG, THE STAR OBSERVED WAS
              NOT DF MON.
DN     MON    MIN II 13.9.
DR     MON    CM./SEE CC MON.
DT     MON    P VAR. MAX=2425324+345D*E (J.D.2425300-28200)
               0387!; B HTEPBAE/IN THE INTERVAL J.D.2429250-
              37700 HAATC K/THERE WERE CYCLES 119D,
              230D, 350D.
DW     MON    B PAOHE PACCEHHOO CKOEH/IN THE REGION
              OF THE OPEN CLUSTER NGC 2286.
EE     MON    P VAR. MAX=2425300.42+4.80776D*E (J.D.2425300-
              27720); OCE/SINCE J.D.2427720-CM. TA./SEE
              TABLE.
EH     MON    D=0.023P.
EK     MON    P VAR. MAX=2425302.59+3.95773D*E (J.D.2425200-
              33000)  0387!; OCE/SINCE J.D.2433000-CM. TA./
              SEE TABLE.
EP     MON    D=0.026P.
ES     MON    D=0.02P.
EW     MON    MIN II 14.2.
FH     MON    CM./SEE AV MON.
FP     MON    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 2353.
FS     MON    MIN II 11.2.
FU     MON    S 6.5/7.5.
FW     MON    D=0.016P. CM./SEE AV MON.
FX     MON    OH MCC/EMISSION.
FZ     MON    EMEHT TPET POBEPK./THE ELEMENTS
              SHOULD BE CHECKED.
GH     MON    MIN II 13.1.
GP     MON    CM./SEE SS MON.
GQ     MON    CM./SEE SS MON.
GR     MON    CM./SEE SS MON.
GU     MON    MIN II 12.5.
GV     MON    CM./SEE AV MON.
GX     MON    OH, H2O, SIO MAEP/MASER.
HI     MON    MIN II 9.9.
HM     MON    MIN II 13.6. P VAR. MIN I=2430110.1948+0.40765737D*E
              (J.D.2429600-35400)  5285!; OCE/SINCE J.D.
              2435400-CM. TA./SEE TABLE.
HO     MON    D=0.03P.
HP     MON    D=0.04P:.
HR     MON    HA MIN II?DEPTH OF MIN II 0.03M.
HY     MON    MIN II 12.4.
IL     MON    D=0.03P.
IM     MON    MIN II 6.47.
IO_IQ  MON    CM./SEE SS MON.
IR     MON    P VAR?
IS     MON    HA MIN II?DEPTH OF MIN II 0.05M.
IX     MON    MIN II 12.8.
IZ     MON    MIN II 12.0.
KU_MN  MON    CM./SEE SS MON.
MO     MON    VB A (B 20M, 10", 356G); CM./SEE SS MON.
MP_MQ  MON    CM./SEE SS MON.
MX     MON    MIN II 11.7.
NN     MON    MIN II 12.9.
NS     MON    MIN II 11.1.
NT_OW  MON    CM./SEE SS MON.
OX     MON    VB A (B 15M, 7", 35G); CM./SEE SS MON.
OY_PQ  MON    CM./SEE SS MON.
PR     MON    CM./SEE FZ MON.
PT_PY  MON    CM./SEE SS MON.
QR     MON    290D<=P<=400D. HA MIN MEHETC HA 0.9M C
              EPOOM OKOO 2000D./DEPTH OF MIN VARIES BY
              0.9M WITH THE PERIOD ABOUT 2000D.
QT_    V346   MON CM./SEE SS MON.
V347   MON    VB A (B 20M, 12", 120G); CM./SEE SS MON.
V348_  V355   MON CM./SEE SS MON.
V356   MON    VB (3", 78G); CM./SEE SS MON.
V357_  V364   MON CM./SEE SS MON.
V365   MON    VB B (A=V591 MON, B 7", 135G); CM./SEE SS MON.
V366_  V367   MON CM./SEE SS MON.
V368   MON    VB (9", 252G); CM./SEE SS MON.
V369   MON    VB (11", 264G); CM./SEE SS MON.
V370   MON    VB (8", 97G); CM./SEE SS MON.
V371   MON    CM./SEE SS MON.
V372   MON    SC 7/7.5.
V373   MON    CM./SEE SS MON.
V379   MON    D=0.015P:.
V380   MON    MIN II 12.9; P=1.98904166D?
V383   MON    MIN II 15.2.
V384   MON    MIN II 13.0.
V389   MON    MIN II 14.9.
V393   MON    MIN II 14.3.
V394   MON    D=0.02P; CM./SEE AV MON.
V395   MON    D=0.03P.
V396   MON    MIN II 13.5.
V397   MON    MIN II 11.9.
V398_  V403   MON CM./SEE SS MON.
V404   MON    D=0.02P:.
V405_  V425   MON CM./SEE SS MON.
V426   MON    VB A (B=NSV 3125 17.0M, 6", 117G); CM./SEE
              SS MON.
V427_  V441   MON CM./SEE SS MON.
V442   MON    MIN II 11.6.
V443_  V444   MON CM./SEE SS MON.
V445   MON    MIN II 11.3.
V446   MON     A/H!=-0.7.
V447   MON     A/H!=-1.4.
V448   MON    MIN II 9.8.
V449   MON    D=0.02P.
V450   MON    MIN II 12.6.
V451   MON    MIN II 14.7.
V452   MON    MIN II 12.7; D=0.02P.
V453   MON    MIN II 11.8.
V454   MON    MIN II 12.2.
V455   MON    MIN II 15.3.
V456   MON    MIN II 13.7.
V457   MON    MIN II 14.3; D=0.03P:.
V458   MON    MIN II 13.8.
V459   MON    MIN II 14.7.
V460   MON    MIN II 10.7.
V463   MON    D=0.03P; P=2.2476768D?
V464   MON    MIN II 12.3.
V465   MON    P VAR. MAX=2429642.44+2.71341D*E (J.D.2425600-
              30800)  3551!; MAX=2431845.65+2.713212D*E (J.D.
              2430000-35200)  3453!; MAX=2435541.315+
              +2.713668D*E (J.D.2435200-41600); OCE/SINCE
              J.D.2441600-CM. TA./SEE TABLE.
V466   MON    VB A (B 15M, 135G).
V474   MON    (K-B)2=0.32. EKT AKO/BLAZHKO EFFECT:
              MAX(O-C)=2441664.962+7.74639D*N; MIN(O-C)=
              =2441669.569+7.74639D*N; 0.03M<=A<=0.37M; -0.02D<=
              <=O-C<=+0.03D.
              ACTOTH AHA BBET TP OCHOBHX KOEA-
              H  8669!:/FREGUENCY ANALYSIS GIVES THREE PRIN-
              CIPAL OSCILLATIONS  8669!: P1=0.1361258D (A1=0.18M),
              P2=0.1337745D (A2=0.12M), P3=0.1385591D (A3=
              =0.04M).
V478_  V479   MON B PAOHE TMAHHOCT/IN THE REGION OF THE
              NEBULA IC 2169.
V481_  V483   MON CM./SEE V478 MON.
V486   MON    VB A (B 18.4M, 6"). CM./SEE V487 MON.
V487_  V489   MON B PAOHE TMAHHOCT/IN THE REGION OF THE
              NEBULA NGC 2245.
V490   MON    B PAOHE TMAHHOCT/IN THE REGION OF THE NEBULA
              NGC 2247.
V493   MON    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER TR 5.
V494   MON    CM./SEE IS MON.
V496   MON    MIN II 12.8.
V497   MON    8.9-11.8 IR.
V498   MON    P=2.4727818D?
V500   MON    CM./SEE SS MON.
V501   MON    MIN II 13.1; MIN II-MIN I=0.445P; DII=0.036P.
V503   MON    9.2-10.9 IR.
V505   MON    MIN II 7.55.
V507   MON    SB2 (P=53.781D  9483!); D=0.015P:.
V510   MON     A/H!=-0.1.
V513   MON    CM./SEE AV MON.
V514   MON    MIN II 13.3.
V515   MON    MIN II 12.7.
V521   MON    MIN II 10.4.
V524   MON    MIN II 15.2.
V526   MON    P VAR. MAX=2433304.284+2.675208D*E (J.D.2429300-
              35170); OCE/SINCE J.D.2439170-CM. TA./SEE
              TABLE.
V527   MON    CM./SEE IS MON.
V530   MON    MIN II 12.8.
V532   MON    MIN II 12.8. RRC?
V535   MON    P VAR. MAX=2431846.445+0.3328791D*E (J.D.
              2429600-34060); OCE/SINCE J.D.2434060-CM.
              TABL>?SEE TABLE.
               FE/H!=-1.44.
V539   MON    CM./SEE CT MON.
V540_  V542   MON CM./SEE VY MON.
V543_  V549   MON CM./SEE CT MON.
V550   MON    VB A (B 17.3M, 6", 0G); CM./SEE CT MON.
V551_  V557   MON CM./SEE CT MON.
V560   MON    CM./SEE IS MON.
V565   MON    CBAHA C HO TMAHHOCT NGC 2313 A-
              METPOM 10"  CO CAO KOMETOOPAHO TMAH-
              HOCT./CONNECTED WITH THE DIFFUSE NEBULA
              NGC 2313 HAVING DIAMETER OF 10" AND A FAINT COME-
              TARY NEBULA.
V569   MON    VB A (B 10.8M, 6.2", 281G; C 10.5M, 38.3", 295G). A-
              H PEE MEHEH CMMAPHOO ECKA KOMO-
              HEHTOB A B./THE RANGE OF COMBINED LIGHT VARIA-
              TION OF A AND B COMPONENTS IS GIVEN.
              COACHO  8215!, /ACCORDING TO  8215!, P=0.18D.
V571   MON    (K-B)2=0.32. HEPAAHE CA, EPO
              KOTOPX MEHTC:/NON-RADIAL PULSATION WITH VA-
              RIABLE PERIODS: P1=0.0999081D (A1=0.052M), P2=
              =0.0749998D (A2=0.015M) (J.D.2440914-41692)
               7127!; P1=0.0894534D (A1=0.038M), P2=0.15988D
              (A2=0.025M), P3=0.106516D (A3=0.014M). P4=0.26998D
              (A4=0.012M), P5=0.15069D (A5=0.011M) (J.D.
              2441662-719)  9450!.
V577   MON    VB (A 11.3M V, B 14.8M V; A=0.312", P=16.60Y, E=
              =0.38); MU ALFA=+0.049S, MU BETA=+0.73". BOMOHO, MEH-
              TC OA KOMOHEHTA. B TAE PBEEH PEE-
               MEHEH CMMAPHOO ECKA CCTEM  6146!./
              BOTH COMPONENTS ARE PROBABLY VARIABLES. THE RANGE
              OF COMBINED LIGHT VARIATION OF THE SYSTEM IS GIVEN
              IN THE TABLE  6146!.
V578   MON    CM./SEE CT MON.
V579_  V586   MON CM./SEE SS MON.
V588_  V589   MON CM./SEE SS MON.
V590   MON    VB (10", 358G); CM./SEE SS MON.
V591   MON    VB A (B=V365 MON, 7", 135G); CM./SEE SS MON.
V593_  V612   MON CM./SEE SS MON.
V613   MON    S 3/2.
V616   MON    HOBOOOHE BCK OTMEEH B 1917 . (MAX
              J.D.2421540)  B 1975 . (MAX J.D.2442646). B
              COKOHOM COCTOH HAAETC, O-BMOM,
              COAHA EPEMEHHOCT C P=0.325D  A=
              =0.2M  9458!, A TAKE OEE MEEHHE MEHEH
              ECKA C P=7.39D  9459!  7.8D  9460!. OCAHE
              CEKTPA  9461, 9462!./NOVALIKE OUTBURSTS WERE OB-
              SERVED IN 1917 (MAX J.D.2421540) AND IN 1975 (MAX
              J.D.2442646). IN GUIESCENT STATE PROBABLY ELLIPSOI-
              DAL LIGHT VARIATION IS OBSERVED WITH P=0.325D AND
              A=0.2M  9458!, AND ALSO SLOWER LIGHT VARIATIONS
              WITH P=7.39D  9459! OR 7.8D  9460!. SPECTRUM DESCRIP-
              TION  9461, 9462!.
V624   MON    CM./SEE CC MON.
V628_  V629   MON CM./SEE SS MON.
V630   MON    VB A (B 21M, 3", 300G); CM./SEE SS MON.
V632   MON    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 2368.
V637   MON    HA OCHOBHOE KOEAHE C A1=0.05M, EMEHT KO-
              TOPOO PBEEH B TAE, HAKABAETC BTO-
              POE C A2=0.02M  EMEHTAM:/BASIC OSCILLATION
              WITH A1=0.05M AND ELEMENTS GIVEN IN THE TABLE IS
              SUPERIMPOSED BY THE SECOND ONE WITH A2=0.02M AND
              THE ELEMENTS: MAX=2443496.1624+0.19740D*E.
              EPO EH/BEAT PERIOD PB=6.09D.
V638   MON    VB (6.5M, 8.5M; 0.8", 178G).
V640   MON    CM./SEE CT MON. PORB=14.39604D  6103!.
              HEPABHE MEHEH ECKA. BOMOHO, EPE-
              XOHA CTA OT BOHO CCTEM O-BE K C-
              CTEME TA WR  4107!./IRREGULAR LIGHT VARIATIONS.
              PROBABLY TRANSITIONAL STAGE FROM A BINARY SYSTEM OF
              O STARS TO A SYSTEM OF WR TYPE  4107!.
V641   MON    VB A (B 10.91M, 21.4", 310G; C 12.46M, 25.8", 285G).
              CM./SEE SS MON. HA MIN II?DEPTH OF MIN II
              0.07M.
V642   MON    CM./SEE SS MON. HE EH CKOEH./CLUSTER NON-
              MEMBER. AHA OXA MIN ECKA./EPOCH OF LIGHT
              MINIMUM IS GIVEN IN THE TABLE.
V645   MON    AHA OXA MIN ECKA./EPOCH OF LIGHT MINIMUM
              IS GIVEN IN THE TABLE.
S      MUS    OTMEEHA HA KAPTE  BO MUS./MARKED ON THE
              CHART FOR BO MUS. MAX II=MAX I,  (MAX II)=0.15P.
              P VAR? SB 1 (PORB=506.4D).
T      MUS    P2=1021D.
V      MUS    B OACT OHOO MEKA./IN THE COAL SACK
              REGION.
RV     MUS    P=128D: BOMOEH/IS POSSIBLE.
RW     MUS    P=130D: BOMOEH/IS POSSIBLE.
RY     MUS    V1 (NGC 4833).
RZ     MUS    V2 (NGC 4833). HE EH CKOEH./CLUSTER NON-
              MEMBER.
SY     MUS    MIN II 11.2; MIN I-MIN II=170D. AH EMEHT
               MIN I HAABXC B HTEPBAE J.D.
              2434910-41510 KBAEPOECKX MEHEH.
              PAOCTOHK./ELEMENTS FOR MIN I OF GUASIPERIO-
              DIC VARIATIONS OBSERVED DURING J.D.2434910-41510
              ARE GIVEN. RADIO SOURCE.
TU     MUS    MIN II 8.65. P VAR. MIN I=2424260.396+1.38728D*E
              (J.D.2423900-29300)  0039!; B HTEPBAE/DURING
              J.D.2437380-41900-CM. TA./SEE TABLE.
              OPMA KPBO ECKA/THE LIGHT CURVE SHAPE VAR.
TV     MUS    MIN II 11.3.
TW     MUS    MIN II 12.4.
TZ     MUS    B-V:+1.22, +1.43.
UW     MUS    MIN II 11.9.
UY     MUS    MIN II 12.0.
VW     MUS    MIN II 13.9.
WY     MUS    P VAR. CHCOAH EH:/PERIODIC TERM:
              +0.35D*SIN (0.12G*E).
XZ     MUS    O/BEFORE J.D.2419200 MAX=2412590+113D*E.
AB     MUS    MIN II 13.0.
AS     MUS     A/H!=0.5.
AX     MUS    P VAR. B HTEPBAE/DURING J.D.2412550-19200-
              CM. TA./SEE TABLE; B HTEPBAE/DURING J.D.
              2423900-26100 P=97.3D.
AY     MUS    MIN II 10.8. MIN II-MIN I=0.481P. EMEHT OB-
              ETBOPT HAEHM B HTEPBAE 1897-1943.
              B HTEPBAE J.D.2441683-721 ATMEH HE HACT-
                8094!./THE ELEMENTS ARE VALID DURING 1897-
              1943. IN THE TIME INTERVAL J.D.2441683-721 EC-
              LIPSES DID NOT OCCUR  8094!.
BB     MUS    P, BOMOHO, CEET BOT./POSSIBLY P SHOULD
              BE DOUBLED.
BD     MUS    HA/DEPTH OF MIN II 0.05M.
BE     MUS    MIN II 14.1.
BF     MUS    MIN II 14.4.
BK     MUS    P OEH OO:/VERY LONG P: 56D<D<310D.
BR     MUS    MIN II 11.25. B-V: +0.10M.
BS     MUS    MIN II 11.5.
BX     MUS    HA/DEPTH OF MIN II 0.04M.
CD     MUS    MIN II 14.7.
CS     MUS    P>120D.
DW     MUS    COACHO  8135!, CEKTP M5E, XAPAKTEPH 
              BE TA MP. EMEHT   3934! BBEEH
              O HAABMC MEHEHM ECKA C P-355D,
              HTEPPETPOBABMC KAK OH EPO: CT-
              PE MEHEH OTBEPEH OTOPAECKM
              HAEHM HA POTEH 7H./ACCORDING TO
               8135!, THE SPECTRAL TYPE IS M5E, TYPICAL OF MIRA
              STARS. ELEMENTS IN  3934! WERE DEDUCED FROM THE OB-
              SERVED BRIGHTNESS VARIATIONS WITH P-355D WHICH
              WAS CONSIDERED TO BE A SPURIOUS PERIOD; RAPID VARIA-
              TIONS WERE CONFIRMED BY 7H OF PHOTOGRAPHIC OBSER-
              VATIONS.
DZ     MUS    CM./SEE BB MUS.
EE     MUS    B OHOM MEKE. BCKA HAAAC CEKT-
              PAHO./IN THE COAL SACK. THE FLARE WAS OBSERVED
              SPECTROSCOPICALLY.
EN     MUS    D=0.035P:.
EP     MUS     A/H!=0.2. COACHO/ACCORDING TO  8136!, EA,
              P=4.15D, D=0.05P, 11.63M-12.60M V, MIN II 11.7:.
ET     MUS    BOMOEH TAKE T/ALTERNATIVELY POSSIBLE TYPE
              EW  8727, 4001!.
EV     MUS    D=0.09P:.
EY     MUS    CM./SEE V MUS.
EZ     MUS    HE CKEH HAEH P/ALTERNATIVE POSSIBLE
              VALUES OF P 4.3032D, 4.3224D.
FH     MUS    HA/DEPTH OF MIN II 0.03M.
FO     MUS    P VAR?
GK     MUS    MIN II 15.0.
GN     MUS    MIN II 14.2.
GO     MUS    MIN II 15.2.
GP     MUS    B-V:+1.03, +1.61.
ALFA   MUS    VB A (B 13.0M, 29.3", 316G).
ETA    MUS    VB A (B 7.30M, 60").
TETA   MUS    VB (A 5.64M, B 7.5M, 5.3", 187G); SB (PORB=18.341B).
              EPEMEHHOCT HTEHCBHOCT MCCOHHX H
              O OTHOEH K KOHTHM (BOHA BOHA; E-
              MEHT B TAE -  OX MIN I). PEMEHHOCT
              B  AX (LAMBDA LAMBDA 1550-3300 A) C AMTO-2%,
              P=1.5D  CTPE MEHEH (LAMBDA LAMBDA 1550-1800 A) C
              AMTO-3-5%  XAPAKTEPHM BPEMEHEM
              50S-70S  8532!./ VARIABLE INTENSITY OF EMISSION
              LINES WITH RESPECT TO THE CONTINUUM (DOUBLE WAVE;
              ELEMENTS IN THE TABLE ARE FOR THE EPOCHS OF MIN I
              VARIABILITY IN THE UV RANGE (LAMBDA LAMBDA 1550-3300 A) WITH
              AN AMPLITUDE ABOUT 2%, P=1.5D AND RAPID CHANGES
              (LAMDA LAMDA 1550-1800 A) WITH AN AMPLITUDE ABOUT 3-5% ON
              THE TIME SCALE OF 50S-70S  8532!.
              CBAHA C TMAHHOCT / CONNECTED WITH A NEBULA,
              80'*45'.
R      NOR    VB A (B 14.0M, 5.7", 268G, 1929). P VAR. MAX II =
              =2406371+486.94D*E (J.D.2406300-25000); MAX II =
              =2426359+500.56D*E (J.D.2426000-30500); MAX II =
              =2431377+489.0D*E (J.D.2430500-34500); OCE/
              SINCE J.D.2437600-CM. TA./SEE TABLE.
              OOHO R CEN, MEET BOHO MAX, PAEEHH
              CPABHTEHO HEOKM MIN II. MAX II OHO
              PE,  EM MAX I./LIKE R CEN,  HAS A DOUDLE MAX,
              DIVIDED BY A COMPARATIVELY SHALLOW MIN II. MAX II IS
              USUALLY BRIGHTER THAN MAX I.  (MIN I)=0.43P,
               (MAX I)=0.70P, (MIN II)=0.85P.
S      NOR    B EHTPE PACCEHHOO CKOEH NGC 6087, EH
              CKOEH./IN THE CENTRE OF THE OPEN CLUSTER
              NGS 6087, CLUSTER MEMBER.
               A/H!=-0.1.
T      NOR    P VAR.MAX=2414783+241.87D*E (J.D.2414700-
              28000); MAX=2428084+244.93D*E (J.D.2428000-
              35000); OCE/SINCE J.D.2437000-CM. TA./SEE
              TABLE.
U      NOR    P VAR. MAX=2415028.94+12.64084D*E (J.D.2415000-
              26000)  0060!; OCE/SINCE J.D.2434000-CM. TA./
              SEE TABLE,   A/H!=-0.6.
W      NOR    P2-1300D.
Y      NOR    VB A (B 12.2M VIS, 4.0", 156G, 1903).
Z      NOR    MIN II 9.6.
RR     NOR    MIN II 9.9.
RS     NOR    B-V:+1.13, +1.48.
RT     NOR    KBAEPOECKE KOEAH:/QUASIPERIODIC VARIA-
              TIONS: P1-59D, P2-175D  8140!.
RV     NOR     A/H!=0.8. KPBA ECKA MEET HEPABHOCT./
              THERE ARE IRREGULARITIES IN THE LIGHT CURVE.
SV     NOR    MIN II 12.6.
SW     NOR    D=0.003P.
SX     NOR    D=0.1P.
SY     NOR    VB A (B 12.8M, 2.1", 315G, 1934). B-V:+1.16, +1.49.
               A/H!=0.5.
SZ     NOR    MIN II 12.6.
TT     NOR    BOMOEH BBOE O P./TWICE LONGER P IS
              POSSIBLE.
TU     NOR    MIN II 12.5. CBAHA C MAEHKO CAO TMAH-
              HOCT./ASSOCIATED WITH A SMALL FAINT NEBULA.
TV     NOR    MIN II 9.3.
TW     NOR    B OACT EHOO PACCEHHOO CKOEH./IN THE
              REGION OF THE POOR OPEN CLUSTER LYNGA 6. B-V:+1.79,
              +2.22.  A/H!=0.2.
TX     NOR    MIN II 12.5.
TZ     NOR    MIN II 12.1.
UV     NOR    D=0.07P.
UX     NOR    B MAX ECKA/IN MAX LIGHT B-V=+0.30.
UY     NOR    D=0.025P.
UZ     NOR    D=0.02P.
VV     NOR    B OACT CKOEH/IN THE REGION OF THE CLUSTER
              NGC 6152.
VX     NOR    HA/DEPTH OF MIN II-0.03M.
VZ     NOR    CM./SEE VV NOR.MIN II 14.3.
WX     NOR    KAPTA OOHO OTMEEHA KAK OTHOCAC K
              WZ NOR./THE CHART IS ERRONEOUSLY LABELLED AS THAT
              FOR WZ NOR. MIN II 12.8.
WZ     NOR    KAPTA OOHO OTMEEHA KAK OTHOCAC K
              WX NOR./THE CHART IS ERRONEOUSLY LABELLED AS THAT
              FOR WX NOR. MIN II 13.4.
XY     NOR    MIN II 13.2.
AA     NOR     A/H!=-0.1.
AF     NOR    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 5999.
AT     NOR    D=0.026P:.
BE     NOR    MIN II 14.2.
BH     NOR    MIN II 13.2.
BP     NOR    K CTHK./CLOSE COMPANION.
CE     NOR    D=0.05P. MIN II 11.8?
CX     NOR    MIN II 15.0.
DO     NOR    MIN II 14.2. CM./SEE DR NOR.
DR     NOR    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6087.
EM     NOR    MIN II 13.8.
ET     NOR    D=0.032P.
FK     NOR    MIN II 15.0.
FQ     NOR    COACHO/ACCORDING TO  0060!, P=1.994D?
FW     NOR    MIN II 14.5.
GM     NOR    D=0.02P; MIN II 11.01; MIN II-MIN I=0.499P
              (J.D.2441683-721), MIN II-MIN I=0.531P (J.D.2425381-
              28402). B-V=0.44M.
GN     NOR    MIN II 13.3, DII=0.16P, MIN II-MIN I=0.405P
              (J.D.2425900). OPTAHOE BEHE:/APSIDAL MO-
              TION: P=500YR.
GO     NOR    MIN II 13.7.
GQ     NOR    MIN II 13.8.
GR     NOR     A/H!=0.9.
GT     NOR    D=0.048P.
GU     NOR    CM./SEE IS NOR. B-V: +1.17, +1.40.  A/H!=0.1.
GV     NOR    D=0.03P:.
GX     NOR    MIN II 15.0.
HH     NOR    VB B (A 9.9M VIS, FO; B 12.6", 148G). D=0.05P.
HI     NOR    D OEH MAO./D IS VERY SMALL.
HK     NOR    MIN II 12.9.
HO     NOR    MIN II 13.2:.
HW     NOR    D=0.024P.
HZ     NOR    P=2.921584D BOMOEH/IS POSSIDLE.
IQ     NOR    B-V: +1.55, +1.93.
IS     NOR    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6067.
IT     NOR    MIN II 9.8.
KL     NOR    P>=140D.
KM     NOR    P>=170D.
KQ     NOR    HE CKEH T MP KTA/MIRA CETI TYPE IS NOT
              EXCLUDED  4001!.
KT     NOR    P>=180D.
KX     NOR    MIN II 14.8.
LO     NOR    P>=220D.
LV     NOR    OK/DEEP MIN II.
LX     NOR    BOMOHE HAEH P:/POSSIBLE P VALUES:
              0.60492D, 0.7851D, ETC.
NR     NOR    MIN II 15.9.
NW     NOR    P>140D.
NX     NOR    MIN II 14.4.
OS     NOR    AHA OXA MIN. BOMOEH T EW/KW./EPOCH OF
              MIN IS GIVEN. EW/KW TYPE IS POSSIBLE.
OT     NOR    MIN II 13.7.
OU     NOR    MIN II 15.1.
OV     NOR    P>=200D.
OW     NOR    P>=120D.
OX     NOR    P>=110D.
PQ     NOR    BOMOHO,  EEA,  BAC OEE CAM
              KOMOHEHTOM HEPAPEEHHO BOHO. AHA OXA
              MAX./POSSIBLY A CEPHEID WHICH IS A FAINTER COMPO-
              NENT OF AN UNRESOLVED BINARY. EPOCH OF MAX IS GIVEN.
PT     NOR    CM./SEE IS NOR.
QV     NOR    3U 1538-52. NO.12  4124!. AHA OXA MIN, COOTBET-
              CTBEO PEHTEHOBCKOM ATMEH. HA
              MINI 0.05M V, HA MIN II 0.08M V. EPO PEHT-
              EHOBCKX MCOB PX=528.928S  4114!. HAA-
              AC BCKA C DM>0.3M  9456!./EPOCH OF MIN COR-
              RESPONDING TO THE X-RAY ECLIPSE IS GIVEN. DEPTH
              OF MIN I 0.05M V, THAT OF MIN II 0.08M V. THE PERI-
              OD OF X-RAY PULSES PX=528.928S  4114!. A FLARE
              WAS OBSERVED WITH DM>0.3M  9456!.
OX     NOR    4U 1608-52.
QZ     NOR    B PACCEHHOM CKOEH/IN THE OPEN CLUSTER
              NGC 6067.
MU     NOR    B OACT PACCEHHOO CKOEH/IN THE REGI-
              ON OF THE OPEN CLUSTER NGC 6169.
U      OCT    P VAR. MAX=2420685+302.00D*E (J.D.2414900-
              20700); MAX=2424320+300.74D*E (J.D.2422800-
              29800); MAX=2431901+309.60D*E (J.D.2429800-
              32250); MAX=2434018+300.70D*E (J.D.2432250-
              38800); OCE/SINCE J.D.2438800 - CM.TA./
              SEE TABLE.
X      OCT    P VAR.MAX=2415170+208.40D*E (J.D.2415100-
              17100); MAX=2417425+201.24D*E (J.D.2417100-
              20700); MAX=2423780+207.95D*E (J.D.2422000-
              24000); MAX=2424370+200.18D*E (J.D.2424000-
              25600); OCE/SINCE J.D.2425600-CM.TA./
              SEE TABLE. HA MIN CHO MEHETC/
              DEPTHS OF MINIMA APE STONGLY VARIABLE;
              1.1M<=A<=4.0M.
RV     OCT    DS=10.
TX     OCT    MIN II 12.7.
UV     OCT    DS=9; (K-D)2=0.06. EKT AKO:/BLAZHKO
              EFFECT: P=80D; 0.14P<=M-M<=0.24P, 0.4M<=A<=1.3M.
UZ     OCT    MIN II 9.48; DI=0.00P, DII=0.05P. P VAR.MIN I=
              =2440223.1560+1.1493709*E (J.D.2438300-
              42000); OCE/SINCE J.D.2442000 - CM.TA./
              SEE TABLE.
AM     OCT    MIN II 14.9.
BE     OCT    P<20D:.
BG     OCT    P=0.7490D?
BK     OCT    MIN II 14.6.
BP     OCT    (K-B)2=0.25.
CC     OCT    HA OCHOBH PAAH CA C P1=0.12490D
              (A1=0.042M) HAKABATC PE C EPOAM:/
              BASIC RADIAL PULSATION WITH P1=0.12490D (A1=0.042M)
              IS SUPERIMPOSED DY OTHERS WITH PERIODS: P2=0.0795317D
              (A2=0.008M), P3=0.12336D (A3=0.014M); P4=
              =0.11068D (A4=0.008M), P5=0.12713D (A5=0.006M);
              P6=0.11815D (A6=0.006M).
CD     OCT    MU=0.51", P=279G. OH  EPOOB/ONE OF THE PE-
              RIODS P=686S (A=0.01M).
CE     OCT    HA KOEAHE ECKA C P2=0.054511D (A2=0.0056M)
              HAKABAETC KOEAHE C P1=0.2100D  0.2660D
              (A1=0.0052M), KOTOPOE MOET T OCOBEHO
               CAE,  COAHO EPEMEHHO-
              CT B TECHO BOHO CCTEME./LIGHT OSCILLATION
              WITH P2=0.054511D (A2=0.0056M) IS SUPERIMPOSED
              DY AN OSCILLATION WITH P1=0.2100D OR 0.2660D (A1=
              =0.0052M), WHICH IS DUE TO PULSATION OR ELLIPSOIDAL
              VARIABILITY IN A CLOSE BINARY SYSTEM.
R      OPH    P VAR.MAX=2399214+302.1D*E (J.D.2399200-2427900)
               0458!; MAX=2427915+304.0D*E (J.D.2427900-34900);
              MAX=2434906+301.5D*E (J.D.2434900-40600)  0001!;
              OCE/SINCE J.D.2440600-CM.TA./SEE TABLE.
U      OPH    ADS 10428 A (B 12.26M, GOV, 20.4", 358G). MIN II 6.46.
              P VAR. EPOECK EH:/PERIODIC TERM:+0.0120D*
              *SIN (0.0483G*E+4.7833G).
V      OPH    P VAR. MAX=2411155+296.73D*E (J.D.2411000-24000);
              MAX=2424198+302.46D*E (J.D.2424000-28000); OCE/
              SINCE J.D.2428000-CM.TA./SEE TABLE.
W      OPH    P VAR. O/BEFORE J.D.2420500 MAX=2415186+
              +335.07D*E; MAX=2420870+325.33D*E (J.D.2420500-
              24700); OCE/SINCE J.D.2424700-CM.TA./SEE
              TABLE.
X      OPH    VBA (A=0.34", PORB=485.3 YR; B-9M, K1III, 0.4", 142G,
              1980). AH PEE MEHEH CMMAPHOO EC-
              KA./THE RANGE OF THE COMBINED BRIGHTNESS IS GIVEN.
              P VAR. MAX=2416416+336.61D*E (J.D.2416400-26000);
              MAX=2426161+331.28D*E (J.D.2426000-32500); MAX=
              =2432788+335.50D*E (J.D.2432500-38000); OCE/
              SINCE J.D.2438000-CM.TA./SEE TABLE.
Y      OPH    SB1? PORB=2612D? P VAR. O/BEFORE J.D.2427000
              MAX=2408694.77+17.11884D*E; OCE/SINCE
              J.D.2432000-CM.TA./SEE TABLE.  A/H!=-0.2.
Z      OPH    P VAR.MAX=2411896+349.0D*E (J.D.2411800-21000)
               0458!; MAX=2420962+352.1D*E (J.D.2421000-25000);
              MAX=2425183+347.4D*E (J.D.2425000-31000); CPEHE
              EMEHT OCE/MEAN ELEMENTS AFTER J.D.2431000-
              CM.TA./SEE TABLE.
RR     OPH    P VAR. KBAPATH EH:/NONLINEAR TERM:
              -0.009282D*E2.
RS     OPH    PEE BCK/PREVIOUS OUTBURSTS: 1898,
              1933, 1958. COACHO  7575!, B 1972-1973 - O-
              PABHE KOEAH/ACCORDING TO  7575!, IN
              1972-1973 THERE WERE SEMIREGULAR VARIATIONS (DM-
              0.5M, P=50D-70D).
RT     OPH    P VAR. O/BEFORE J.D.2426500 MAX=2417452+
              +429.00D*E; MAX=2426461+422.67D*E (J.D.2426500-
              34000); OCE/SINCE J.D.2434500-CM.TA./SEE
              TABLE. OH, H2O MAEP/MASER.
RU     OPH    P VAR. O/BEFORE J.D.2422000 MAX="$ '#((+
              +200.95D*E; MAX=2422011+203.62D*E (J.D.2422000-
              27300); MAX=2427298+200.5D*E (J.D.2427300-29000);
              MAX=2429305+203.88D*E (J.D.2429000-33000); B H-
              TEPBAE/DURING J.D.2433000-40500-CM.TA./SEE
              TABLE.
RV     OPH    D=0.015P; MIN II 9.56, DII=0.09P. OPMA KPBO EC-
              KA/THE LIGHT CURVE SHARE VAR.
RW     OPH    P VAR. MAX=242494+247.86D*E (J.D.2425000-34000).
              B TAE AH CPEHE EMEHT./THE TABLE GIVES
              MEAN ELEMENTS.
RX     OPH    OH, H2O MAEP/MASER.
RY     OPH    P VAR. MAX=2415235+151.05D*E (J.D.2414700-24000);
              MAX=2424152+149.69D*E (J.D.2424000-31000); MAX=
              =2431339+150.94D*E (J.D.2431000-40000); OCE/
              SINCE J.D.2440000-CM.TA./SEE TABLE.
RZ     OPH    D=0.030P.
SS     OPH    P VAR. O/BEFORE J.D. 2432500 MAX=2417330+
              +179.88D*E.
ST     OPH    (K-B)2=0.03.
SV     OPH    EMEHT CPABEB OCE/THE ELEMENTS ARE VALID
              SINCE J.D. 2422000.
SW     OPH    VB A (B 12.0MVIS, 2.4", 91G, 1943). D=0.02P. P VAR.
              MIN=2418880.528+2.445948D*E (J.D. 2418880-26200)
               0001!; MIN=2431235.216+2.446086D*E (J.D. 2427900-
              33500)  2389!; OCE/SINCE J.D. 2434000- CM.TA./
              SEE TABLE.
SX     OPH    D=0.03P.
SZ     OPH    P VAR. O/BEFORE J.D. 2428400 MIN=2421057.556+
              +3.708454D*E; OCE/SINCE J.D. 2442000 - CM.TA./
              SEE TABLE.
TT     OPH     FE/H!=-0.5.
TW     OPH    P2=2000D:. CBAHA C TMAHHOCT EPEMEHHO
              PKOCT/ASSOCIATED WITH A NEBULA OF VARIABLE BRIGHT-
              NESS  3479!.
UU     OPH    D=0.024P. P VAR?
UX     OPH    P VAR. MAX=2426041+117.34D (J.D. 2406430-28040);
              OCE/SINCE J.D. 2433100 - CM.TA./SEE TABLE.
VW     OPH    P VAR. AH CPEHE EMEHT./MEAN ELEMENTS ARE
              GIVEN. B HTEPBAE/DURING J.D. 2422500-30600
              MAX=2430554+282.69D*E.
WW     OPH    AHA OXA MIN./EPOCH OF MIN IS GIVEN.
WZ     OPH    MIN II 9.82.
XX     OPH    CMOTECK O'EKT,  XAPAKTEPC O-
              KM POOTEHM OCAEHM ECKA
               9489!./A SYMBIOTIC OBJECT FEATURING DEEP FADINGS
              OF LONG DURATION  9489!.
AH     OPH    H2O MAEP/MASER.
BF     OPH    SB? P VAR? OCE/SINCE J.D. 2430000 - CM.TA./
              SEE TABLE.
BN     OPH    80D=<P=<250D.
DM     OPH    P VAR. P=220D (1893-1910), P=216D (1914-1928).
DQ     OPH    P=35D BOMOEH/IS POSSIBLE.
FK     OPH    V2 (NGC 6273).
GM     OPH    V12 (NGC 6284).
GR     OPH    P VAR. MAX=2415425+136D*E (1893-1908); B HTEP-
              BAE/DURING 1910-1928 - CM.TA./SEE TABLE.
IL     OPH    P2=140D:.
IW     OPH    B OACT APOBOO CKOEH NGC 6293, BOMO-
              H EH CKOEH./IN THE FIELD OF THE GLOBULAR
              CLUSTER NGC 6293, POSSIBLE CLUSTER MEMBER.
KM     OPH    B OACT APOBOO CKOEH NGC 6304, BEA
              O./IN THE FIELD OF THE GLOBULAR CLUSTER NGC 6304,
              FIELD STAR.
KO     OPH    B TEMHO TMAHHOCT./IN A DARK NEBULA.
KQ     OPH    P2=1500D.
KR     OPH    P2>5000D.
OU     OPH    V70 (NGC 6266).
PU     OPH    VB (A=V29 (NGC 6266), AHHE B TAE/THE DATA
              ARE IN THE TABLE; B=V28 (NGC 6266), 16.6M-17M, 4B,
              4.8", 7G), B: RRAB, MAX=2433423.52+0.49749D*E,
              M-M=0.15P.
V378   OPH    MIN II 14.2. B OACT PACCEHHOO CKOEH
              CR 359. AHA OXA MAX./IN THE REGION OF THE OPEN
              CLUSTER CR 359. EPOCH OF MAX IS GIVEN.
V380   OPH    PORB=0.16D. OA./BLUE.
V391   OPH    CM./SEE V 423 OPH. P VAR? O/BEFORE J.D. 2427000
              MIN=2425501.425+2.89558D*E  0432!; OCE/SINCE
              J.D. 2441500 - CM.TA./SEE TABLE.
V392   OPH    KPACHA./RED.
V402   OPH    P VAR. MAX=2425364+154D*E (J.D. 2425350-670);
              OCE/SINCE J.D. 2425670 - CM.TA./SEE TABLE.
V413   OPH    DS=3. EKT AKO?/BLAZHKO EFFECT?
V414   OPH    B-V:+0.41, +0.77.
V423   OPH    B OACT PACCEHHOO CKOEH./IN THE REGION OF
              THE OPEN CLUSTER CR 359.
V426   OPH    BCK C HTEPBAAM 17D-55D  8079!; B 1976-77
              K 32.3D. BHE BCK 12.7M-13.3M, BOH C K-
              OM 20-30 MH  OEE MEEHHE KOEAH./OUT-
              BURSTS SEPARATED BY 17D-55D  8079!; IN 1976-77 THE
              CYCLE WAS 32.3D. OUTSIDE OUTBURSTS 12.7M-13.3M, WA-
              VES WITH A CYCLE OF 20-30 MIN AND SLOWER VARIATIONS.
V438   OPH    H20 MAEP./MASER.
V439   OPH    B-V:+0.63, +0.97.
V442   OPH    PORB=0.14056D.
V445   OPH    VB A (B 13.04MY, 21"NF). (K-B)2=0.35; DS=2. COA-
              CHO/ACCORDING TO  5692!, EKT AKO/BLAZH-
              KO EFFECT (>2000D).
V449   OPH    P VAR. O/BEFORE J.D. 243900 MIN=2428696.465+
              +1.243078D*E; MIN=2442959.607+1.243095*E
              (J.D. 2439000-43000); OCE/SINCE J.D. 2443000 -
              CM.TA./SEE TABLE.
V451   OPH    MIN II 8.31; MIN II-MIN I=0.494P; DII=0.12P.
V452   OPH    DS=5:.
V455   OPH    P VAR? AH CPEHE EMEHT, HAEC B
              OTBEPEH./THE TABLE GIVES MEAN ELEMENTS
              WHICH NEED CONFIRMATION.
V456   OPH    MIN II 10.5. P VAR. O/BEFORE J.D. 2436100 MIN=
              =2428422.341+1.015986D*E  0476!; OCE/SINCE
              J.D. 2441800 - CM.TA./SEE TABLE.
V465   OPH    B-V:+0.68, +1.10. P VAR?
V471   OPH    OEH KPACHA./VERY RED.
V478   OPH    B-V:+0.86, +1.33.  A/H!=-0.7. EMEHT HAT-
              C B OTBEPEH./THE ELEMENTS NEED CONFIRMATI-
              ON.
V487   OPH    D=<0.14P. CM./SEE V 423 OPH.
V496   OPH    CM./SEE V 423 OPH.
V501   OPH    MIN II 11.1.
V502   OPH    MIN II 8.81. P VAR. OCE/SINCE J.D. 2434500 - CM.
              TA./SEE TABLE.
V506   OPH    MIN II 12.0. CM./SEE V 423 OPH.
V508   OPH    MIN II 10.59.
V509   OPH    CM./SEE V 423 OPH.
V511   OPH    MIN II 13.7. CM./SEE V 423 OPH.
V515   OPH    MAX=2425600+300D*E (J.D. 2425600-26700); P=
              =140D (J.D. 2426700-27300); B HTEPBAE/DURING
              J.D. 2427300-30200 - CM.TA./SEE TABLE.
V516-V 517OPH B OACT APOBOO CKOEH/IN THE REGION
              OF THE GLOBULAR CLUSTER NGC 6304.
V521   OPH    P=164D (J.D. 2415000-24600); P2-4000D.
V526   OPH    MIN II 13.6.
V527   OPH    MIN II 14.8.
V532   OPH    P>=6000D.
V533   OPH    P>=80D.
V534   OPH    D=0.03P.
V535   OPH    D=0.025P.
V536   OPH    D=0.04P:.
V537   OPH    MIN II 12.8.
V540   OPH    D=0.05P; MIN II 13.4.
V541   OPH     A/H!=-1.0. B OACT APOBOO CKOEH
              NGC 6401; HE EH CKOEH?/IN THE REGION OF THE
              GLOBULAR CLUSTER NGC 6401; CLUSTER NON-MEMBER?
V543   OPH    MIN II 13.6.
V549   OPH    MIN II 14.0.
V550   OPH    MIN II 13.0.
V554   OPH     A/H!=-1.1.
V555   OPH    OCTPE  TE MAX. EKT AKO?/SHARP AND
              FLAT MAXIMA. BLAZHKO EFFECT?
V557   OPH    MIN II 15.7. CM./SEE V 423 OPH.
V558   OPH    B-V:+0.57, +0.68.  FE/H!=-1.48. COACHO/ACCOR-
              DING TO  9037!, P=0.299D.
V564   OPH     FE/H!=-1.37. AHA OXA MIN./EPOCH OF MIN IS
              GIVEN. P VAR. KBAPATH EH:/NONLINEAR TERM:
              +0.0073D*(E+10)**2.
V565   OPH    P=0.3957D BOMOEH/IS POSSIBLE. OTOEKTPEC-
              KE HAEH 1968 POTBOPEAT EMEHTAM
               5746!./PHOTOELECTRIC OBSERVATIONS OF 1968 CONTRADICT
              THE ELEMENTS  5746!.
V566   OPH    DI=0.048P; MIN II 7.89, DII=0.06P. P VAR. O/BEFORE
              J.D. 2440500 MIN=2436744.4200+0.40964091D*E
               8287!; OCE/SINCE J.D. 2440500 - CM.TA./SEE
              TABLE.
V567   OPH    (K-B)2=0.22;DS=0. COACHO/ACCORDING TO  7984!,
              MAX=2441134.467+0.1300729D*E.
V568   OPH    KPACHA./RED.
V570   OPH    VB A (B 16.3M, 5", 90G).
V572   OPH    CM./SEE V 423 OPH.
V573   OPH    D=0.034P. CM./SEE V 423 OPH.
V574   OPH    P2-500D.
V577   OPH    MIN II 11.9. MIN II-MIN I=0.583P. DII=0.050P. E=0.22.
V580   OPH    VB A (B 15.5M, 0.2').
V585   OPH    HAKABAETC OOEPOECKOE KOEAHE?/
              A LONG-PERIOD VARIATION IS SUPERIMPOSED?
V586   OPH    CM./SEE V 423 OPH.
V590   OPH    MIN II 13.6.
V592   OPH    MAX=2427227+78D*E (J.D. 2426100-29400); B H-
              TEPBAE/DURING J.D. 2429400-30150 - CM.TA./SEE
              TABLE. OCE HTEPBAOB HEPABHO EPEMEHHO-
              CT EPOHOCT BOCCTAHABBAETC E CBA
              A./AFTER INTERVALS OF IRREGULAR VARIABILITY THE PERI-
              ODICITY RESUMES WITHOUT PHASE SHIFT.
V605   OPH    CM./SEE WW OPH.
V618   OPH    MIN II 14.7:.
V636   OPH    D=0.030P.
V683   OPH    P VAR. OPMA KPBO ECKA MEHETC./THE LIGHT
              CURVE SHAPE VARIES.
V687   OPH    BOMOHO, P BBOE HHEE./P MAY BE TWICE LONGER.
V693   OPH    EKT AKO?/BLAZHKO EFFECT?  5692!.
V695   OPH    P VAR? OPMA KPBO ECKA MEHETC./THE LIGHT
              CURVE SHAPE VARIES.
V698   OPH    P VAR? OCE/SINCE J.D. 2442950 - CM.TA./SEE TABLE.
V700   OPH    B-V:+0.49, +0.50.  FE/H!=-2.10.
V716   OPH    DS=7.
V720   OPH    VI (NGC 6171). HE EH CKOEH./CLUSTER NON-
              MEMBER.
V722   OPH    P VAR. MAX=2437089.456+0.6190385D (J.D. 2419900-
              37100)  7806!; OCE/SINCE J.D. 2436700 - CM.TA./
              SEE TABLE.
V729   OPH    P VAR. MAX=2437492.766+0.4685794D*E (J.D. 2423500-
              37800)  3560!; OCE/SINCE J.D. 2437400 - CM.TA./
              SEE TABLE.
V732   OPH    HEOHA KPBA ECKA (OCTP MAX; ABH
              MIN; POK MAX;BTOPH MIN 15.2)./UNUSUAL
              LIGHT CURVE (SHARP MAX; PRIMARY MIN; BROAD MAX; SE-
              CONDARY MIN 15.2).
V734   OPH    P VAR. MAX=2420636.497+0.562489D*E (J.D. 2420600-
              29100); B HTEPBAE/DURING J.D. 2429100-37150 -
              CM.TA./SEE TABLE.
V735   OPH    MIN II 10.6.
V737   OPH    P=374D BOMOEH/IS POSSIBLE.
V767   OPH    COACHO  0104!, BOH C DM=0.3M-1.4M VIS PO-
              OTEHOCT 50D-110D; CPEH BEHA VAR,
              DM-0.4M B TEEHE 800D-:1000D./ACCORDING TO
               0104!, WAVES WITH DM=0.3M-1.4M VIS OF 50D-110D
              DURATION; MEAN BRIGHTNESS VAR, DM-0.4M IN 800D-
              -1000D.
V782   OPH    OEH KPACHA./VERY RED.
V784   OPH    B-V:+0.26, +0.56. EPO HAETC B POBEPKE./
              THE PERIOD SHOULD BE CHECKED.
V786   OPH    KPACHA./RED.
V788   OPH    CM./SEE V822 OPH. =115D.
V799   OPH    P=215D BOMOEH/IS POSSIBLE.
V802   OPH    KPACHA./RED.
V816   OPH    B-V:+0.25, +0.63.
V8222  OPH    EKT AKO?/BLAZHKO EFFECT?
V823   OPH    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER IC 4665.
V825   OPH    CM./SEE V823 OPH.
V829   OPH    CM./SEE V822 OPH. =165D.
V832   OPH    KPACHA./RED.
V838   OPH    P2-500D BOMOEH/IS POSSIBLE.
V839   OPH    MU=0.041", RO=292G. MIN II 9.38.
V840   OPH    VB A (B 12M, 16", 116G).
V841   OPH    MAX=2396146.
V843   OPH    SN KEPLER. MAX 2307193. AOB OCTATOK./GASE-
              OUS REMNANT.
V844   OPH    MIN II 14.9.
V845   OPH    VB A (B 15.7M).
V847   OPH    MIN II 13.1.
V848   OPH    MIN II 13.4.
V851   OPH    MAX=2425828+95D*E (J.D. 2425600-29700); B H-
              TEPBAE/DURING J.D.2429700-34250 - CM.TA./
              SEE TABLE.
V854   OPH    COACHO  8116!, CEKTP HAOMHAET  CEKTP BE-
               TA TTAU./ACCORDING TO  8116!, THE SPECTRUM
              RESEMBLES THAT OF A TTAU-TYPE STAR.
V868   OPH    MIN II 13.6. CM./SEE V423 OPH.
V870   OPH    CM./SEE V823 OPH.
V872   OPH    P=0.825D BOMOEH/IS POSSIBLE.
V878   OPH    MIN II 16.5. CM./SEE V423 OPH.
V911   OPH    P2=81D, P3=114D. P4>P3? OCTAHOBK O 100D./
              STANDSTILLS UP TO 100D.
V919   OPH    VB A (B SP).
V920   OPH    MIN II 15.9.
V924   OPH    MIN II 16.4.
V929   OPH    D=0.050P.
V934   OPH    BOMOEH T E./E TYPE IS POSSIBLE.
V936   OPH    CM./SEE V823 OPH.
V938   OPH    MIN II 15.3. CM./SEE V423 OPH.
V940   OPH    MIN II 15.6.
V941   OPH    MIN II 16.5.
V943   OPH    MIN II 16.4. CM./SEE V423 OPH.
V945   OPH    MIN II 15.1. CM./SEE V423 OPH.
V947   OPH    MIN II 14.5. CM./SEE V423 OPH.
V952   OPH    P=0.954D BOMOEH./IS POSSIBLE.
V954   OPH    CM./SEE V423 OPH. MIN II 14.9. COACHO/ACCORDING
              TO  3500!, CONST, V=12.86M, B-V=+1.36M,
V959   OPH    P VAR? MAX=2429785.419+0.084857D*E
              (J.D. 2429785-845)  2757!; B HTEPBAE/DURING
              J.D. 2443719-732 - CM.TA./SEE TABLE; BOMO-
              H TAKE EMEHT:/OTHER POSSIBLE ELEMENTS: MAX=
              =2443726.469+0.07786D*E.
V960   OPH    CM./SEE V423 OPH.
V963   OPH    MIN II 15.1. CM./SEE V423 OPH.
V968   OPH     FE/H!=-1.48. CM./SEE V423 OPH.
V969   OPH    MIN II 13.8:. CM./SEE V423 OPH.
V977-V 978OPH B OACT APOBOO CKOEH/IN THE REGION
              OF THE GLOBULAR CLUSTER NGC 6426.
V979   OPH    V11 (NGC 6426). HE EH CKOEH./CLUSTER NON-
              MEMBER.
V980   OPH    CM./SEE V977 OPH. P=0.25740D BOMOEH/IS POSSI-
              BLE.
V983   OPH    CM./SEE V423 OPH.
V986   OPH    B E 1980 . V MEHAC C P=0.179D, 0.147D,
              0.225D , BOMOHO, 0.097D, HO CEKTPAHX ME-
              HEH HE O,  OTOMETPECK P=0.323D B V
              HE POBC. SB? PORB=15D-20D; B OTOMETP-
              ECKX AHHX TAKE MEETC TOK MOHOCT
              HA HKX ACTOTAX. B CCEOBAHX PEHX
              ET OTMEAC OTOMETPECKE EPO 0.284D-
              0.4D  HAPEH EPOHOCT./IN JULY 1980 V
              VARIED WITH P=0.179D, 0.147D, 0.225D, AND POSSIBLY
              0.097D, BUT THERE WERE NO SPECTRUM VARIATIONS, AND
              THE PHOTOMETRIC P=0.323D WAS NOT NOTICEABLE IN V.
              SB? PORB=15D-20D; THERE IS ALSO EXCESS POWER
              AT LOW FREQUENCES IN THE PHOTOMETRIC DATA. EARLIER
              STUDIES REVEALED PHOTOMETRIC PERIODS 0.284D-0.4D
              AND VIOLATION OF PERIODICITY.
V987   OPH    D=0.02P. MIN II 14.6. CM./SEE V423 OPH.
V998-V 999OPH B OACT APOBOO CKOEH/IN THE REGI-
              ON OF THE GLOBULAR CLUSTER NGC 6171.
V1000  OPH    CM./SEE V822 OPH.
V1002  OPH    MIN II 15.2. BOMOEH T RRC C OOBHHM P./
              RRC TYPE WITH TWICE SHORTER P IS POSSIBLE.
V1004  OPH    CM./SEE V822 OPH.
V1010  OPH    MIN II 6.46. P VAR. P=0.661464D (J.D. 2415000-
              25000)  5738!; OCE/SINCE J.D. 2425000 - CM.TA.,
              KBAPATH EH:/SEE TABLE, NONLINEAR TERM:
              -3.87D*10**-10*E**2. OPMA KPBO ECKA  HA
              MIN I VAR./THE LIGHT CURVE SHAPE AND THE DEPTH OF
              MIN I VAR.
V1011  OPH    CM./SEE V822 OPH.
V1015  OPH    D=<0.23P, D<0.02P; MIN II 14.5.
V1017  OPH     FE/H!=-1.25. P VAR? MAX=2437433.935+0.2343D*E
              (J.D. 2437433-514)  3625!. B HTEPBAE/DURING
              J.D. 2442954-45140 - CM.TA./SEE TABLE. COAC-
              HO/ACCORDING TO  9037!, P=0.361D.
V1018  OPH    BOMOHO, ATMEHHA./POSSIBLY ECLIPSING.
V1021  OPH    DM VAR. B-V:+0.42, +0.62.
V1022  OPH    D=0.06P:; MIN II 15.95.
V1024  OPH    MAX=2437433.559+0.5914D*E (J.D. 2437433-514)
               3625!. B HTEPBAE/DURING J.D. 2442954-45140 -
              CM.TA./SEE TABLE. BOMOEH T RR(B); P=
              =0.371D OBETBOPET HAEHM B HTEPBAE
              J.D. 2442954-44407./RR(B) TYPE IS POSSIBLE; P=
              =0.371D SATISFIES THE OBSERVATIONS DURING
              J.D. 2442954-44407.
V1026  OPH    MAX=2437433.562+0.6563D*E (J.D.2437433-514)
               3625!. B HTEPBAE/DURING J.D. 2442954-45140 -
              CM.TA./SEE TABLE.
V1028  OPH    CM./SEE V822 OPH.
V1032  OPH    P>1.0D HE CKEH/IS NOT EXCLUDED.
V1033  OPH    MAX=2437433.714+0.4845D*E (J.D. 2437433-514)
               3625!. B HTEPBAE/DURING J.D. 2442954-45140 -
              CM.TA./SEE TABLE.
V1035  OPH    MAX=2437433.388+0.6100D*E (J.D. 2437433-514)
               3625!; B HTEPBAE/DURING J.D. 2442954-45140 -
              CM.TA./SEE TABLE.
V1039  OPH    P=0.3166D BOMOEH/IS POSSIBLE.
V1040  OPH    OPMA KPBO ECKA VAR./THE LIGHT CURVE SHAPE
              VAR.
V1041  OPH     FE/H!=-1.06.
V1042  OPH    CM./SEE V1040 OPH. MAX=2437433.633+0.5528D
              (J.D. 2437433-514)  3625!. B HTEPBAE/DURING
              J.D. 2442954-45140 - CM.TA./SEE TABLE.
V1052  OPH    MAX=2437433.537+0.7546D*E (J.D. 2437433-514)
               3625!; B HTEPBAE/DURING J.D. 2442954-45140 -
              CM.TA./SEE TABLE.
V1054  OPH    VB WOLF 630AB (A 9.76MV, 12.47MU; B 9.78MV; A=
              =0.22", PORB=1.71665 ; C=WOLF 629, 11.70MV,
              14.75MU, DM4, 72", D=VB8, 16.7MV, 221", OEE
              MU/COMMON MU). MU=1.19", RO=222G. LX/LOPT(V)=0.05.
V1072  OPH    P VAR. MAX=2439025.31+0.444715D*E (J.D. 2438500-
              39025); OCE/SINCE J.D. 2442800 - CM.TA./SEE
              TABLE.
V1075  OPH    KPACHA./RED.
V1077  OPH    P VAR. MAX=2438614.40+0.373926D*E (J.D. 2438200-
              700); MAX=2442871.516+0.37384D*E (J.D. 2442810-
              910): MAX=2442983.345+0.373911D*E (J.D. 2442920-
              3330); OCE/SINCE J.D. 2443330 - CM.TA./SEE
              TABLE.
V1089  OPH    VB AB (B 16.4M, 2", 45G).
V1099- V1100O PH KPACHA./RED.
V1111  OPH    OH, H2O, SIO MAEP/MASER.
V1120  OPH    MIN II 14.3.
V1121  OPH    MK PEHTEHOBCK CTOHK./SOFT X-RAY SOUR-
              CE.
V1135  OPH     CA/H!=-0.74.
V1141- V1142O PH P VAR? OPMA KPBO ECKA/THE LIGHT
              CURVE SHAPE VAR?
V1146  OPH    P=185.2D BOMOEH/IS POSSIBLE.
V1153  OPH    P=153.0D BOMOEH/IS POSSIBLE.
V1157  OPH    B-V:+0.42, +0.66.
V1161  OPH    P=0.49D BOMOEH/IS POSSIBLE  6438!.
V1168  OPH    CM./SEE V1141 OPH.
V1170  OPH    P=360D: BOMOEH/IS POSSIBLE  6438!.
V1174  OPH    CM./SEE V1141 OPH.
V1176  OPH    P=269.0D BOMOEH/IS POSSIBLE.
V1179  OPH    CM./SEE V1141 OPH.
V1185  OPH    BOMOH TAKE EMEHT:/OTHER POSSIBLE ELE-
              MENTS: MAX=2435630+177D*E  0001!.
V1195  OPH    EE OH/ONE MORE MAX 2435637 (1956). BOMO-
              EH T M./TYPE M IS POSSIBLE.
V1203  OPH    P=315D BOMOEH/IS POSSIBLE  6438!.
V1204  OPH    P=144D: /OR P=191D: BOMOH/ARE POSSI-
              BLE.
V1235  OPH    BOMOEH T UV./UV TYPE IS POSSIBLE.
V1240  OPH    P=0.42136D BOMOEH/IS POSSIBLE.
V1244  OPH    CM./SEE V1141 OPH.
V1258  OPH    P VAR?
V1261- V1262O PH KPBA ECKA HE XAPAKTEPHA  P B
              TAE/THE LIGHT CURVE IS NOT TYPICAL
              FOR THE P IN THE TABLE  6438!.
V1276  OPH     CA/H!=-0.1.
V1296  OPH     CA/H!=-0.9.
V1299  OPH    CM./SEE V1141 OPH.
V1300  OPH    P=235D: BOMOEH/IS POSSIBLE.
V1305  OPH    MIN II 17.9:.
V1307  OPH    CM./SEE V1141 OPH. KAC EPO?/SPU-
              RIOUS PERIOD?  6438!.
V1323  OPH    P VAR?
V1332  OPH     CA/H!=-0.64.
V1348  OPH    CM./SEE V1141 OPH.
V1355  OPH    CM./SEE V1141 OPH.
V1403  OPH    P=215D?
V1423  OPH    CM./SEE V1141 OPH.
V1426  OPH    P VAR?
V1451  OPH    P=179.4D?
V1474  OPH    P=127D:?
V1491  OPH    P=328.0D?
V1492  OPH    CM./SEE V1141 OPH.
V1505  OPH    P=86D:?
V1512  OPH    CM./SEE V1141 OPH.
V1526  OPH    P=0.29745D?
V1532  OPH    P=144.4D?
V1534  OPH    P=198.8D?
V1554  OPH    P=136.0D?
V1568  OPH    P=275.5D?
V1571  OPH    P VAR?
V1573  OPH    T/TYPE E?
V1583  OPH    P - KAC?/SPURIOUS?
V1616  OPH    T/TYPE E?
V1628  OPH    CM./SEE V1141 OPH.
V1637  OPH     CA/H!=-0.44.
V1661  OPH    CM./SEE V1141 OPH.
V1666  OPH    P=154.2D?
V1676  OPH    TECH OTECK CTHK?/CLOSE OPTICAL COMPA-
              NION?
V1682  OPH    P=118.0D?
V1687  OPH    T/TYPE CW?
V1702  OPH    P=121D?
V1705  OPH    P VAR?
V1710  OPH    P=0.37422D?
V1731  OPH    CM./SEE V1141 OPH.
V1736  OPH    P=143.8D?, P=244.5D?
V1744  OPH    P=191.6D?
V1748  OPH    A VAR. T/TYPE CW?
V1754  OPH    P=128.4D?
V1768  OPH    CM./SEE V1141 OPH.
V1775  OPH    T/TYPE EW?
V1793  OPH    P=170D:?
V1803  OPH    HE EHTHA C 438./THE STAR IS NOT SVS 438.
V1805  OPH    CM./SEE V1141 OPH.
V1811  OPH    MIN II 17.9:.
V1814  OPH    P=160.4D?
V1822  OPH    P VAR?
V1829  OPH    P=143.2D?
V1840  OPH    V 12 (NGC 6333=M9). EH CKOEH./CLUSTER
              MEMBER.
V1841  OPH    CM./SEE V1141 OPH.
V1845  OPH    V7 (NGC 6333=M9). EH CKOEH./CLUSTER
              MEMBER.
V1853  OPH    CM./SEE V1141 OPH.
V1860  OPH     CA/H!=-0.49.
V1861  OPH    P=142.0D?
V1864  OPH    V3 (NGC 6333=M9). EH CKOEH./CLUSTER
              MEMBER.
V1886  OPH    CM./SEE V1141 OPH.
V1889  OPH    P=316.0D?
V1895  OPH    CM./SEE V1141 OPH.
V1905  OPH    P=149.0D?
V1919  OPH    P=102.8D?, P=227.0D?
V1939  OPH    P=330.0D?
V1946  OPH    CM./SEE V1141 OPH.
V1952  OPH    P=248.0D?
V1953  OPH    P=199D:?, P=235D:?
V1954  OPH    P=159.6D?
V1973  OPH    P=0.24154D?
V1989  OPH    A VAR?
V1990  OPH    P=121D:?
V1991  OPH    CM./SEE V1141 OPH.
V1994  OPH    P=170.0D?
V1998  OPH    P=270.5D?
V2002  OPH    CM./SEE V1141 OPH.
V2003  OPH     CA/H!=-0.96.
V2009  OPH    V5 (NGC 6356). EH CKOEH./CLUSTER MEMBER.
V2010  OPH     CA/H!=-0.79.
V2016  OPH     CA/H!=-0.96.
V2042  OPH    P VAR. MAX=2430146.478+0.5385D*E (J.D. 2429100-
              30202); OCE/SINCE J.D. 2436700 - CM.TA./SEE
              TABLE.
V2048  OPH    SB 2  6598!. CM./SEE V423 OPH. HAP C HEPA-
              BHM KOEAHM ECKA, THM 
              BE-BE, HAATC CTPE BCK C AM-
              TO O 1.8M (LAMBDA EFF=5800 A)  6150!. HE CK-
              EHO, TO BCK POCXOT HA OEE CAOM
              CTHKE CCTEM./ALONG WITH IRREGULAR LIGHT VARI-
              ATIONS TYPICAL FOR BE STARS THERE ARE RAPID FLARES
              WITH THE AMPLITUDES UP TO 1.8M (LAMBDA EFF=5800 A)
               6150!. IT IS NOT EXCLUDED THAT THE FLARES OCCUR ON A
              FAINTER COMPANION OF THE SYSTEM.
V2051  OPH    OHO - 15.0M C CHM KTAM ECKA
              (O 0.4M A 5 MHT)  PEKM BCKAM. B TO
              E BPEM HAATC ATMEH HO O
              2.5M C EMEHTAM:/USUALLY - 15.0M WITH STRONG FLI-
              CKERING OF BRIGHTNESS (UP TO 0.4M IS 5 MINUTES) AND
              RARE FLARES. AT THE SAME TIME THE ECLIPSES ARE OB-
              SERVED WITH DEPTH TO 2.5M WITH THE ELEMENTS: MIN=
              =2444787.32124+0.062427865D*E  9550!; D=
              =0.0088P:, D=0.0065P.
V2058  OPH    B TEMHO TMAHHOCT B OACT RO OPH./IN THE
              DARK NEBULA IN THE RO OPH REGION.
V2059  OPH    CM./SEE V2058 OPH.
V2061  OPH    B OACT APOBOO CKOEH./IN THE REGION OF
              THE GLOBULAR CLUSTER NGC 6171 (M 107).
V2062- V2064O PH CM./SEE V2058 OPH.
V2101  OPH    B TEMHO TMAHHOCT./IN A DARK NEBULA.
V2102  OPH    B PAOHE APOBOO CKOEH./IN THE REGION OF
              THE GLOBULAR CLUSTER NGC 6293.
V2105  OPH    V=100 KM/C.
V2106  OPH    <V>=-102 KM/C.
V2108  OPH    H2O, SIO MAEP/MASER.
V2112  OPH    HA OCHOBHOE KOEAHE C A1=0.0172M (CM.TA.)
              HAKABAETC BTOPOE (A2=0.0061M) C EMEHTA-
              M:/THE PRIMARY OSCILLATION WITH A1=0.0172M
              (SEE TABLE) IS SUPERIMPOSED BY THE SECONDARY ONE
              (A2=0.0061M) WITH THE ELEMENTS: MAX=
              =2444114.531:+0.1449461D*E.
V2116  OPH    X-CAP. EPO MCOB MEHAETC:
              135S (1971 .), 112.076S (1979 .), 109.668S (1980 .)
               9553!. EPO BPAEH MOET T BBOE
              OE./X-RAY PULSAR. THE PULSE PERIOD IS DEC-
              REASING: 135S (1971), 112.076S (1979), 109.668S
              (1980)  9553!. THE SPIN-PERIOD MAY BE TWICE
              LONGER.
V2118  OPH    BOMOHO, CTPO BPAAAC OHOHA F -
              BEA C THAM. AHA OXA MAX ECKA./PRO-
              BABLY RAPIDLY ROTATING SINGLE SPOTTED F TYPE STAR.
              MAX BRIGHTNESS EPOCH IS GIVEN.
V2119  OPH    B PAOHE APOBOO CKOEH NGC 6284. HE EH
              CKOEH./IN THE REGION OF THE GLOBULAR CLUSTER
              NGC 6284. NOT A MEMBER OF THE CLUSTER.
V2120  OPH    V6 (NGC 6284). CM./SEE V2119 OPH.
V2121  OPH    V10 (NGC 6284). CM./SEE V2119 OPH.
V2122  OPH    CM./SEE V2119 OPH.
V2123  OPH    V11 (NGC 6284). CM./SEE V2119 OPH.
V2124  OPH    CM./SEE V2119 OPH.
TETA   OPH    SB 1 (PORB=11.44D  6597!). HA OCHOBHOE KOEAHE
              (CM.TA.) HAKABATC KOEAH C EPOA-
              M:/THE BASIC OSCILLATION (SEE TABLE) IS SUPERIM-
              POSED BY OSCILLATIONS WITH THE PERIODS: P1=0.092551D,
              P2=0.069452D, P3=0.0555D, P4=0.0464D, P02=
              =0.137255D, P13=0.13845D, P24=0.13990D, P03=
              =0.09185D.
HI     OPH    SB 1 (PORB=138.8D  9558!).
OMEGA  OPH    P=1.5D?
R      ORI    SC 5/9.5 E. P VAR. MAX=2399420+378D*E (J.D.
              2395600-99500); MAX=2412687+378.1D*E (J.D.
              2403200-12700); MAX=2414230+366.5D*E (J.D.
              2413800-16800); MAX=2417943+378.1D*E (J.D.
              2416800-21350); MAX=2421352+384.9D*E (J.D.
              2421350-24100); OCE/SINCE J.D. 2424100 - CM.
              TA./SEE TABLE.
S      ORI    VB A (B 10.9M, 47", 228G). SIO MAEP/MASER. P VAR.
              MAX=2404538+412.00D*E (J.D. 2404520-13600);
              MAX=2414014+427.15D*E (J.D. 2414000-19150);
              MAX=2419567+416.11D*E (J.D. 2419570-22890);
              MAX=2423312+407.10D*E (J.D. 2423320-31050);
              MAX=2431454+438.53D*E (J.D. 2431500-39000)
               3765!; OCE/SINCE J.D. 2439000 - CM.TA./SEE
              TABLE.
T      ORI    B T-ACCOA TMAHHOCT OPOHA. CBAHA C
              KOMETOOPAHO TMAHHOCT./IN THE T-ASSOCIA-
              TION OF THE ORION NEBULA. CONNECTED WITH A COMETA-
              RY NEBULA.
U      ORI    SIO, OH, H2O MAEP/MASER. P VAR. MAX=2409881+
              +374.5D*E (J.D. 2409800-15900); MAX=2415871+
              +367.9D*E (J.D. 2415900-21000); MAX=2421016+
              +376.0D*E (J.D. 2421000-29300); MAX=2428164+
              +368.3D*E (J.D. 2428100-32900)  0960!; MAX=
              +2433336+372.7D*E (J.D. 2432900-43800); OCE/
              SINCE J.D. 2443800 - CM.TA./SEE TABLE.
V      ORI    P VAR. MAX=2413656+264.8D*E (J.D. 2411800-18700);
              MAX=2418987+271.7D*E (J.D. 2418700-24600);
              MAX=2424695+263.7D*E (J.D. 2424600-29400)
               0960!; MAX=2430769+269.9D*E (J.D. 2430700-
              36200); OCE/SINCE J.D. 2437700 - CM.TA./SEE
              TABLE.
W      ORI    CPEH BEHA MEHETC C P=2450D./MEAN
              MAGNITUDE VARIES WITH P=2450D.
Z      ORI    MIN II 9.9; D=0.013P.
RS     ORI    P VAR. MAX=2428073.205+7.566836D*E (J.D. 2416500-
              33000); OCE/SINCE J.D. 2435000 - CM.TA./SEE
              TABLE.
RT     ORI    CPEH BEHA MEHETC C P=3200D./MEAN
              MAGNITUDE VARIES WITH P=3200D.
RU_RW  ORI    B PAOHE TMAHHOCT IC 434./IN THE REGION OF
              THE NEBULA IC 434.
RX     ORI    B PAOHE  T-ACCOA TMAHHOCT OPOHA./IN
              THE REGION OF THE ORION NEBULA T-ASSOCIATION.
RZ_TW  ORI    CM./SEE RX ORI.
TX     ORI    VB A (B=TY ORI, 42.4", 45G); CM./SEE RU ORI.
TY     ORI    VB B (A=TX ORI); CM./SEE RU ORI.
TZ     ORI    CM./SEE RU ORI.
UW     ORI    MIN II 11.6.
UY_UZ  ORI    CM./SEE RX ORI.
VV     ORI    MIN II 5.50; DI=0.055P; DII=0.064P. B CCTEME ME-
              ETC TPET KOMOHEHT/THE IS THIRD COMPONENT
              IN THE SYSTEM (PORB=119.09D  8045!).
VW_VX  ORI    CM./SEE RX ORI.
VY     ORI    VB A (B=16.6MV, 16", 135G). CM./SEE RX ORI.
VZ_WW  ORI    CM./SEE RX ORI.
WX     ORI    VB A (B 17M, 11", 10G). CM./SEE RX ORI.
WY_XY  ORI    CM./SEE RX ORI.
XZ     ORI    BOMOHA EPOHOCT B MEHEHX ECKA./
              THE PERIODICITY IN LIGHT VARIATIONS IS POSSIBLE. CM./
              SEE RX ORI.
YY     ORI    OH MCC/EMISSION. CM./SEE RX ORI.
YZ_AF  ORI    CM./SEE RX ORI.
AG     ORI    VB A (B 16.4MV, 16", 185G). CM./SEE RX ORI.
AH_AL  ORI    CM./SEE RX ORI.
AM     ORI    VB A (B 20.3MV, 3.5", 320G). CM./SEE RX ORI.
AN_AQ  ORI    CM./SEE RX ORI.
AR     ORI    VB A (B 2", 240G). CM./SEE RX ORI.
AS_AU  ORI    CM./SEE RX ORI.
AV     ORI    VB A (B 18.7MV, 6", 305G). CM./SEE RX ORI.
AW_BF  ORI    CM./SEE RX ORI.
BG     ORI    CM./SEE RU ORI.
BH     ORI    CM./SEE RX ORI.
BK     ORI    P VAR. MAX=2422016+338.0D*E (J.D. 2413550-22100);
              MAX=2428880+326.5D*E (J.D. 2422300-28880);
              MAX=2429940+345.3D*E (J.D. 2428880-29940);
              MAX=2432892+327.7D*E (J.D. 2429940-32900);
              MAX=2438800+346.3D*E (J.D. 2432900-38800);
              OCE/SINCE J.D. 2438800 - CM.TA./SEE TABLE.
BM     ORI    CM./SEE RX ORI. B CKOEH/IN THE CLUSTER NGC
              1976. EH TPAE OPOHA:/ORION TRAPEZIUM
              MEMBER: TETA**1 ORI B (A=V1016 ORI; B 8.7", 32G;
              C 5.13M, 13.1", 131G; D 6.70M, 21.6", 96G). D=0.05P;
              MIN II 7.98. OPMA KPBO ECKA  H MH-
              MMOB MEHTC./SHAPE OF THE LIGHT CURVE AND
              DEPTHS OF MINIMA VARY.
BO_BP  ORI    CM./SEE RX ORI.
BS_CH  ORI    CM./SEE RX ORI.
CI     ORI    VB A (B 9.70M, 12.9", 88G).
CM     ORI    P VAR?
CN     ORI    PORB=0.163097D. HA KPB ECKA HAKABATC
              KOEAH, OBETBOPE CEM EMEH-
              TAM:/LIGHT CURVE IS SUPERPOSED BY OSCILLATIONS WITH
              THE FOLLOWING ELEMENTS: MAX0=2444941.5032+
              +0.163097D*E (A0=0.2M), MAX1=2444941.573+
              +0.15946D*E (A1=0.1M)  9471!. HOA HAAT-
              C TAKE OEE CAE CTPE KOEAH C EPO-
              AM OT 24.3S O 29.5S (A<1%)./SOMETIMES SMALLER
              RAPID LIGHT OSCILLATIONS ARE ALSO OBSERVED WITH PERI-
              ODS 24.3S-29.5S (A<1%).
CO     ORI    EH T-ACCOA/MEMBER OF THE T-ASSOCIATION
              CO ORI. VB A (B 13M, 1", 280G).
CP     ORI    MIN II 11.2. P VAR  2545!.
CT     ORI    SRD? P=68D?  9496!.
CW     ORI    MIN II 13.2.
DK     ORI    CM./SEE RX ORI. VB (RO<3").
DL     ORI    CM./SEE RX ORI.
DM     ORI    CM./SEE RX ORI.
DN     ORI    MIN II 9.9; D=0.026P. P VAR. MIN I=2428497.51+
              +12.9649D*E (J.D. 2425200-28600); OCE/SINCE
              J.D. 2435570 - CM.TA./SEE TABLE.
DY     ORI    B-V:+0.58, +1.72.
EG     ORI    D=0.086P. P VAR?
EQ     ORI    MIN II 10.3. P VAR. MIN I=2425889.706+1.74608D*E
              (J.D. 2425600-26700)  2839!; MIN I=2429219.467+
              +1.74611D*E (J.D. 2427700-31000)  0001!; OCE/
              SINCE J.D. 2431000 - CM.TA./SEE TABLE.
ER     ORI    VB A (B 13.6", 0G). MIN II 9.97. P VAR. MIN I=
              =2426336.6485+0.4233955D*E (J.D. 2426330-33920)
               0279!; MIN I=2434765.6306+0.42340620D*E
              (J.D. 2433920-35475)  2278!; MIN I=2436508.7851+
              +0.4234009D*E (J.D. 2435475-40000)  3787!; OCE/
              SINCE J.D. 2440000 - CM.TA./SEE TABLE. OPMA
              KPBO ECKA MEHETC./SHAPE OF THE LIGHT CURVE
              VARIES.
ET     ORI    MIN II 11.3. P VAR?
EW     ORI    MIN II 10.5; MIN II-MIN I=0.529P. B PAOHE PACCEH-
              HOO CKOEH/IN THE REGION OF THE OPEN CLUSTER
              CR 70. B PAOTE  0007! MIN II PHMATC A
              MIN I,  HAOOPOT (MIN II-MIN I=0.47P).  OKOHA-
              TEHOO BOPA OX MIN I HH OTOEKTP-
              ECKE HAEH./IN  0007! MIN II ARE ACCEPTED
              TO BE MIN I, AND VICE VERSA (MIN II-MIN I=0.47P).
              FOR DECISIVE CHOICE OF THE MIN I EPOCH PHOTOELECT-
              RIC OBSERVATIONS ARE NECESSARY. P VAR? MIN II=
              =2429974.810+6.9368005D*E  0007!; OCE/SINCE
              J.D. 2430000 - CM.TA./SEE TABLE.
EY     ORI    MIN II 9.54; D=0.003P. CM./SEE RX ORI. P VAR.
              MIN I=2427310.420+16.787450D*E  0007!; OCE/
              SINCE J.D. 2427500 - CM.TA./SEE TABLE.
EZ     ORI    CM./SEE RX ORI.
FF     ORI    MIN II 10.3.
FH     ORI    D=0.035P. P VAR.
FI     ORI    VB A (B 10.5M, 5", 323G). OPMA KPBO ECKA ME-
              HETC, BOMOHO, EPOECK/SHAPE OF THE LIGHT
              CURVE VARIES, PROBABLY PERIODICALLY  3790, 5475!.
FK     ORI    P VAR. MIN=2427773.390+1.947447D*E (J.D. 2426900-
              37500); OCE/SINCE J.D. 2437500 - CM.TA./SEE
              TABLE.
FL     ORI    P VAR. MIN=2427452.271+1.550971D*E (J.D.2427450-
              29600)  3115!; MIN=2430400.649+1.55093D*E (J.D.
              2429600-30400);MIN=2432517.755+1.550991D*E
              (J.D.2430400-32900); MIN=2434459.571+1.550965D*E
              (J.D.2432900-35050); MIN=2436649.568+1.550995D*E
              (J.D.2435050-40600); OCE/SINCE J.D.2440600 -
              CM.TA./SEE TABLE.
FO     ORI    MIN II 9.7; D=0.005P.
FR     ORI    MIN II 11.1.
FT     ORI    MIN II 9.60; DII=0.08P; MIN II-MIN I=0.73P. P VAR.
              MIN I=2433009.553+3.150404D*E (J.D.2426380-38000)
               2758!; OCE/SINCE J.D.2438000 - CM.TA./SEE
              TABLE. EPO BPAEH H AC 520+-100 ET/
              THE PERIOD OF APSIDAL MOTION 520+-100 YEARS  7358!.
FU     ORI    EH T-ACCOA FU ORI. PACOOEHA B TEMHO
              OE B 35, CBAHA C PKO KOMETOOPAHO T-
              MAHHOCT  PKO BOOPOHO TMAHHOCT S 280.
              MAX ECKA-ETOM 1937 . B 1980 . 10.6M B./MEM-
              BER OF FU ORI T-ASSOCIATION.  IN THE DARK GLOBULE B35.
              CONNECTED WITH A BRIGHT COMETARY NEBULA AND THE BRIGHT
              HYDROGEN NEBULA S 280. LIGHT MAXIMUM WAS IN SUMMER
              1937. IN 1980 - 10.6M B.
FZ     ORI    MIN II 11.2.
GG     ORI    MIN II 11.1; MIN II-MIN I=0.427P.
GP     ORI    SC 7/8-.
GQ     ORI    VB A (B 9.7M, 31", 324G).
GW     ORI    B T-ACCOA/IN THE T-ASSOCIATION CO ORI.
GX_GY  ORI    CM./SEE GW ORI.
GZ_HH  ORI    CM./SEE RX ORI.
HI     ORI    CM./SEE GW ORI.
HK     ORI    CM./SEE GW ORI. CBAHA C PKO KOMETOOPAHO
              TMAHHOCT./CONNECTED WITH A BRIGHT COMETARY NEBU-
              LA. CO, CH, OH MCC/EMISSION.
HL     ORI    CM./SEE RX ORI.
HM     ORI    CM./SEE GW ORI.
HN_LY  ORI    CM./SEE RX ORI.
LZ     ORI    VB B (A 10.3M; B 14.1", 219G). CM./SEE RX ORI.
MM_NT  ORI    CM./SEE RX ORI.
NU     ORI    CM./SEE RX ORI. B TMAHHOCT/IN THE NEBULA NGC
              1982. EBA OOOKA./DUST SHELL.
NV_NX  ORI    CM./SEE RX ORI.
NY     ORI    VB B (A=V566 ORI; B 5", 135G). CM./SEE RX ORI.
NZ_OR  ORI    CM./SEE RX ORI.
OT_PP  ORI    CM./SEE RX ORI.
PQ     ORI    CM./SEE RU ORI.
PR_PT  ORI    CM./SEE RX ORI.
PU     ORI    CM./SEE RU ORI.
PV_PW  ORI    CM./SEE RX ORI.
PX     ORI    <V>=+298 KM/C  9511!. CM./SEE RX ORI.
PY_QQ  ORI    CM./SEE RX ORI.
QR     ORI    B PAOHE T-ACCOA/IN THE REGION OF T-ASSOCIA-
              TION FU ORI.
QT     ORI    P VAR? EMEHT, AHHE B TAE, OBETBOPT
              HAEHM B HTEPBAE/ELEMENTS GIVEN IN THE
              TABLE ARE VALID IN THE INTERVAL J.D.2429640-35550.
V340   ORI    AHA OXA MIN ECKA./EPOCH OF MIN BRIGHTNESS IS
              GIVEN.
V343   ORI    MIN II 11.0. OPMA KPBO ECKA  HA MIN II
              MEHTC./SHAPE OF THE LIGHT CURVE AND DEPTH OF
              MIN II VARY.
V347_  V349   ORI CM./SEE RX ORI.
V353_  V358   ORI CM./SEE RX ORI.
V359   ORI    CM./SEE RX ORI. AHA OXA MIN HTEHCBHOCT -
              H HEI./EPOCH OF MIN HEI LINE INTENSITY IS GIVEN.
              COACHO/ACCORDING TO  9512!, P=14.612D.
V360   ORI    CM./SEE RX ORI.
V361   ORI    VB C (A 4.8M; B 6.1M, 52.4", 93G; C 129", 97G). CM./
              SEE RX ORI.
V362_  V369   ORI CM./SEE RX ORI.
V370   ORI    CM./SEE GW ORI.
V371   ORI    MU=0.28", RO=238G.
V372_  V379   ORI CM./SEE RX ORI.
V380   ORI    B TMAHHOCT/IN THE NEBULA NGC 1999. CM./SEE
              RX ORI. OCAHE CEKTPA/SPECTRUM DESCRIPTION
               4002!. OH, CH MCC/EMISSION.
V381   ORI    CM./SEE RX ORI.
V382   ORI    P VAR. MAX=2431146+227.8D*E (J.D.2429300-31200);
              B TAE PBEEH CPEH EPO/MEAN PERIOD IS
              GIVEN IN THE TABLE (J.D.2428100-33700).
V383_  V391   ORI CM./SEE RX ORI.
V393_  V428   ORI CM./SEE RX ORI.
V432   ORI    DS=0.
V435   ORI    P VAR. MAX=2430350+186D*E (J.D.2429600-30730);
              MAX=2431373+186D*E (J.D.2431370-3250)  2279!;
              OCE/SINCE J.D.2434000 - CM.TA./SEE TABLE.
V436_  V439   ORI CM./SEE GW ORI.
V441   ORI    CM./SEE GW ORI.
V442   ORI    VB A (B 16.6M, 20", 73G). CM./SEE GW ORI.
V443_  V448   ORI CM./SEE GW ORI.
V449   ORI    CM./SEE GW ORI. B PAOTE  8289! OTHECEHA K EPE-
              MEHHM TA EW C EMEHTAM:/IN  8289! WAS CON-
              SIDERED AS AN EW TYPE VARIABLE WITH THE ELEMENTS:
              MIN I=2430259.622+0.441990D*E (J.D.2430250-5550),
              14.8M-15.7M PG.
V450   ORI    CM./SEE GW ORI.
V452_  V458   ORI CM./SEE GW ORI.
V460_  V461   ORI CM./SEE GW ORI.
V463_  V465   ORI CM./SEE GW ORI.
V466   ORI    CM./SEE RX ORI.
V467   ORI    CM./SEE GW ORI.
V468   ORI    CM./SEE RX ORI.
V470   ORI    CM./SEE RX ORI. BEA/STAR  1411. POM/NEAR
              TO WY ORI= 1396.
V473_  V475   ORI CM./SEE RX ORI.
V476_  V477   ORI B PAOHE PACCEHHOO CKOEH/IN THE REGI-
              ON OF THE OPEN CLUSTER LAMBDA)ORI.
V478   ORI    CM./SEE RX ORI.
V479   ORI    CM./SEE RX ORI. B HPAKPACHX AX A>1.5M./
              IN THE INFRARED A>1.5M.
V480   ORI    CM./SEE V479 ORI.
V481_  V482   ORI CM./SEE RX ORI.
V484   ORI    CM./SEE RX ORI. B HPAKPACHX AX A>1.0M./
              IN THE INFRARED A>1.0M.
V485   ORI    CM./SEE V484 ORI.
V486_  V488   ORI CM./SEE RX ORI.
V489_  V491   ORI CM./SEE V484 ORI.
V492   ORI    CM./SEE RX ORI. CEBEPH KOMOHEHT TECHO AP
              HPAKPACHX BE. B HPAKPACHX AX A=1M./
              NORTHERN COMPONENT OF THE CLOSE PAIR OF INFRARED STARS.
              IN THE INFRARED A=1M.
V493   ORI    CM./SEE V484 ORI.
V494   ORI    CM./SEE RX ORI.
V495   ORI    CM./SEE RX ORI. TECHA APA (RO=0.24"). KAKO KOM-
              OHEHT MEHETC, HEBECTHO./CLOSE BINARY (RO=
              =0.24"). IT IS UNKNOWN WHICH OF THE COMPONENTS VARIES.
V496_  V497   ORI CM./SEE V484 ORI.
V498   ORI    CM./SEE RX ORI.
V500_  V502   ORI CM./SEE RX ORI.
V504   ORI    MIN II 15.4.
V505   ORI    CM./SEE RU ORI.
V507_  V511   ORI CM./SEE RU ORI.
V514   ORI    CM./SEE RU ORI.
V516   ORI    MAX=2430325+139D*E (J.D.2430250-5350); P=70D
              (J.D.2435350-550).
V519   ORI    MIN II 12.9.
V522_  V523   ORI CM./SEE RU ORI.
V525   ORI    MIN II 14.7.
V526   ORI    CM./SEE QR ORI.
V529   ORI    NOVA ORI 1678? OBTOPHA BCKA, BOMOHO, HA-
              AAC B 1894  2866!. PAHEE PACCMATPBAAC
              KAK NOVA ORI 1667  2862, 2863, 2867, 2868!, CE-
              CTBOBAHE KOTOPO OCAPBAOC  3813!./RECURRENT
              OUTBURST WAS POSSIBLY OBSERVED AT 1894  2866!. EAR-
              LIER THE OBJECT WAS CONSIDERED AS NOVA ORI 1667
               2862, 2863, 2867, 2868!, ITS EXISTENCE BEING CONSI-
              DERED AS DOUBTFUL  3813!.
V537   ORI    CM./SEE V476 ORI.
V538_  V542   ORI CM./SEE RX ORI.
V544_  V547   ORI CM./SEE RX ORI.
V548_  V549   ORI CM./SEE V476 ORI.
V550_  V557   ORI CM./SEE RX ORI.
V559_  V571   ORI CM./SEE RX ORI.
V572   ORI    CM./SEE V476 ORI.
V573_  V582   ORI CM./SEE RX ORI.
V584_  V594   ORI CM./SEE RX ORI.
V595   ORI    CM./SEE RU ORI.
V596   ORI    CM./SEE V476 ORI.
V597   ORI    CM./SEE RU ORI.
V598   ORI    CM./SEE V476 ORI.
V599   ORI    CM./SEE RX ORI.
V600_  V608   ORI CM./SEE RU ORI.
V610_  V611   ORI CM./SEE RU ORI.
V612   ORI    CM./SEE RU ORI. VB A (B 4.2", 330G).
V614   ORI    CM./SEE QR ORI.
V615_  V623   ORI CM./SEE RU ORI.
V625_  V632   ORI CM./SEE QR ORI.
V634_  V639   ORI CM./SEE QR ORI.
V640   ORI    D=<0.02P.
V641   ORI    MIN II 14.5.
V642   ORI    D=0.05P?.
V643   ORI    P=26.2075D?
V647   ORI    MIN II 11.9. P VAR. MIN I=2418005.035+0.977575D*E
              (J.D.2414660-23230); OCE/SINCE J.D.2423230 -
              CM.TA./SEE TABLE.
V648   ORI    MIN II 12.2.
V649   ORI    CM./SEE GW ORI. VB A (B 15M, 2", 0G).
V650   ORI    CM./SEE V476 ORI.
V652   ORI    CM./SEE RX ORI.
V654_  V659   ORI CM./SEE RX ORI.
V667   ORI    MIN II 15.0.
V676_  V684   ORI CM./SEE RX ORI.
V685   ORI    CM./SEE RX ORI. A(U)=1.0M.
V686_  V712   ORI CM./SEE RX ORI.
V713   ORI    CM./SEE RX ORI. A(U)=4.0M.
V714_  V717   ORI CM./SEE RX ORI.
V718   ORI    CM./SEE RX ORI. O-BMOM, SF-KOMOHEHT OEH
              TECHO BOHO./PROBABLY THE SF-COMPONENT OF A VE-
              RY CLOSE PAIR.
V719_  V736   ORI CM./SEE RX ORI.
V737   ORI    CM./SEE RX ORI. A(U)>2.4M.
V738_  V739   ORI CM./SEE RX ORI.
V740   ORI    CM./SEE RX ORI. A(PG)>4.0M.
V741_  V742   ORI CM./SEE RX ORI.
V744_  V757   ORI CM./SEE RX ORI.
V758   ORI    CM./SEE V740 ORI.
V759_  V766   ORI CM./SEE RX ORI.
V767   ORI    CM./SEE RX ORI. A(U)=1.5M.
V768   ORI    CM./SEE RX ORI.
V770_  V777   ORI CM./SEE RX ORI.
V778   ORI    CM./SEE RX ORI. A(PG)=1.6M.
V779   ORI    CM./SEE RX ORI.
V780   ORI    CM./SEE V685 ORI.
V781_  V782   ORI CM./SEE RX ORI.
V783   ORI    CM./SEE RX ORI. A(PG)=3.0M.
V784_  V806   ORI CM./SEE RX ORI.
V807   ORI    CM./SEE V740 ORI.
V808   ORI    CM./SEE RX ORI.
V810_  V835   ORI CM./SEE RX ORI.
V836   ORI    CM./SEE RX ORI. A(U)>1.5M.
V837   ORI    CM./SEE V740 ORI.
V838_  V839   ORI CM./SEE RX ORI.
V840   ORI    CM./SEE RX ORI. A(PG)=0.7M.
V841_  V854   ORI CM./SEE RX ORI.
V855   ORI    CM./SEE RX ORI. A(U)>2.0M.
V856   ORI    CM./SEE RX ORI.
V857   ORI    CM./SEE RX ORI. A(PG)>5.0M.
V858_  V866   ORI CM./SEE RX ORI.
V867   ORI    CM./SEE RX ORI. A(PG)>3.0M.
V868_  V875   ORI CM./SEE RX ORI.
V876   ORI    CM./SEE RX ORI. H KOMOHEHT TECHO BOHO./
              SOUTHEM COMPONENT OF A CLOSE PAIR.
V877_  V882   ORI CM./SEE RX ORI.
V883   ORI    CM./SEE RX ORI. CBAHA C KOMETOOPAHO TMAH-
              HOCT./IN THE APEX OF A COMETARY NEBULA.
V884_  V885   ORI CM./SEE RX ORI.
V886   ORI    CM./SEE RX ORI. A(PG)>3.5M.
V888_  V891   ORI CM./SEE RX ORI.
V892   ORI    CM./SEE RX ORI. H KOMOHEHT BOHO/SOU-
              THERN COMPONENT OF A PAIR (RO=3").
V893   ORI    CM./SEE RX ORI. A(U)=2.0M.
V894_  V899   ORI CM./SEE RX ORI.
V900   ORI    CM./SEE RX ORI. A(PG)>2.5M.
V901   ORI    CM./SEE RU ORI.
V902   ORI    CM./SEE RX ORI.
V904_  V909   ORI CM./SEE RX ORI.
V916   ORI    P=0.28297D? EH PACCEHHOO CKOEH/MEMBER
              OF THE OPEN CLUSTER NGC 2169.
V917   ORI    EH PACCEHHOO CKOEH/MEMBER OF THE OPEN
              CLUSTER NGC 2169.
V918_  V924   ORI CM./SEE RX ORI.
V926_  V935   ORI CM./SEE RX ORI.
V937_  V939   ORI CM./SEE RX ORI.
V941_  V943   ORI CM./SEE RX ORI.
V945_  V952   ORI CM./SEE RX ORI.
V953   ORI    CM./SEE RU ORI.
V956_  V957   ORI CM./SEE RU ORI.
V958   ORI    CM./SEE RX ORI.
V960   ORI    CM./SEE RU ORI.
V961   ORI    CM./SEE RX ORI.
V964   ORI    P VAR. MAX=2415800.389+0.5046772D*E (J.D.
              2415800-21010); MAX=2424500.446+0.50466477D*E
              (J.D.2424500-30500);  OCE/SINCE J.D.2431500 -
              CM.TA./SEE TABLE.
V965_  V992   ORI CM./SEE RX ORI.
V994_  V997   ORI CM./SEE RX ORI.
V998   ORI    MU=0.28", RO=221G.
V999_  V1002  ORI CM./SEE RX ORI.
V1003  ORI    MU=0.272", RO=60.8G.
V1004  ORI    VB A (B 10.57M, 37", 204G); SB (P=2.74D).
V1005  ORI    B TAE PBEEH PEE MEHEH EC-
              KA ME BCKAM, XAPAKTEPHE  EPE-
              MEHHOCT TA BY DRA; AMTA BCEK
              A(U) MOET OCTAT 3.2M./THE RANGE OF LIGHT
              VARIATIONS (CHARACTERISTIC FOR BY DRA TYPE VARIA-
              BULUTY) BETWIIN THE FLARES IS GIVEN IN THE TABLE;
              THE AMPLITUDE OF THE FLARES A(U) CAN REACH 3.2M.
V1006_ V1007  ORI CM./SEE RX ORI.
V1016  ORI    CM./SEE RX ORI. B CKOEH/IN THE CLUSTER NGC
              1976. EH TPAE OPOHA:/ORION TRAPEZIUM
              MEMBER: TETA1 ORI A (B=BM ORI, 8.7", 32G; C 5.13M,
              13.1", 131G; D 6.70M, 21.6", 96G). D=0.001P.
V1017_ V1020  ORI CM./SEE RX ORI.
V1022  ORI    CM./SEE QR ORI.
V1028  ORI    P=6D?
V1029  ORI    CM./SEE RX ORI.
V1030  ORI    CM./SEE RU ORI. VB (SIGMA ORI) E (A 4.1M; B 5.1M, A=
              =0.247", P=170Y; C 8.79M, 11.2", 238G; D 6.66M,
              12.9", 84G; E 41.6", 61G). MIN I (HEI)=2442802.48+
              +1.19080D*E. HEOHA EEBA EPEMEHHA. B TA-
              E AHA OXA MIN I ECKA (MIN II 6.71, MIN II-MIN I=
              =0.43P), HACTAA HA 0.18P OE OX MH-
              MMA HTEHCBHOCT H HEI LAMBDA 4026 A. COAC-
              HO  9524!, MHMM ECKA OCOBEH "ATME-
              HM" OBEPXHOCT BE BM BOOPOHO-E-
              EBM OAKAM, PACOOEHHM B OT PO-
              TBOOOHX OTHOCTEHO EHTPA BE OA-
              CTX B EPECEEH EE OHOO  MAHTHO-
              O KBATOPOB./UNUSUAL HELIUM VARIABLE. EPOCH OF
              MIN I BRIGHTNESS IS GIVEN IN THE TABLE (MIN II 6.71,
              MIN II-MIN I=0.43P). THIS EPOCH IS BEING OBSERVED
              BY 0.18P LATER THAN THE EPOCH OF MINIMUM STRENGTH
              OF THE HEI LAMBDA 4026 A LINE. ACCORDING TO  9524!, LIGHT
              MINIMA ARE DUE TO "ECLIPSES" OF THE STAR SURFACE
              BY TWO ISOLATED CLOUDS (CONSISTING OF HYDROGEN AND
              HELIUM), WHICH ARE LOCATED ALMOST OPPOSITELY NEAR
              THE INTERSECTIONS OF THE MAGNETIC AND ROTATIONAL
              EQUATOR.
V1031  ORI    VB (0.159", 104G, 1980.7). MIN II 6.32; DII=0.017P.
V1034  ORI    AHA OXA MIN ECKA./EPOCH OF LIGHT MINIMUM
              IS GIVEN.
V1035_ V1045  ORI CM./SEE RX ORI.
V1046  ORI    CM./SEE RX ORI. SB 1. MIN II 6.58. MOET T,
              COAHA EPEMEHHA, HA KOEAH EC-
              KA KOTOPO HAKABATC MEHEH ECKA
              ABHOO KOMOHEHTA, OTHOCEOC K T
              SX ARI: MIN (HEI)=2442812.23+0.9015D*E  8054!./
              POSSIBLY AN ELLIPSOIDAL VARIABLE, ITS LIGHT VARIATIONS
              BEING SUPERIMPOSED BY LIGHT VARIATIONS OF THE
              PRIMARY COMPONENT OF SX ARI TYPE: MIN (HEI)=
              =2442812.23+0.9015D*E  8054!.
V1047_ V1050  ORI CM./SEE RX ORI.
V1052_ V1053  ORI CM./SEE RX ORI.
V1054  ORI    CM./SEE V1034 ORI. P=8.596D?, P=8.674D?
V1055  ORI    P(X)=5.2D  9528!.
V1056  ORI    VB A (B 9.8M, 28.7", 58G).
V1058_ V1084  ORI CM./SEE RX ORI.
ALFA   ORI    VB A (B 14.5M, 39.8", 110G). MIN=2410600+2070D*E
              (1840-1929)  1012!. OCE/SINCE 1929 - CM.TA./
              SEE TABLE. HA ABHOE KOEAHE HAKABATC
              BOH C P=200-400D. AOBO-EBA OOOKA/
              THE MAIN VARIATION IS SUPERIMPOSED BY THE WAVES
              WITH P=200-400D. DUST-GASEOUS SHELL (R=50")
               9529!.
DELTA  ORI    VB A (A 0.217", 144G, 1980; B 14.0M, 33.1", 227G;
              C 6.84M, 53.5", 359G). CM./SEE EPSILON ORI. MIN II 2.20.
              BEHE H AC/APSIDAL MOTION (P=210 YR).
              OPMA KPBO ECKA MEHETC. BOMOHA -
              ECKA EPEMEHHOCT ECKA KOMOHEHTOB./SHAPE
              OF THE LIGHT CURVE VARIES. THE INTRINSIC BRIGHTNESS VA-
              RIABILITY OF THE COMPONENTS IS POSSIBLE.
EPSILO ORI    EH CKOEH OC OPOHA./ORION BELT CLUSTER
              MEMBER.
ETA    ORI    VB AAB (AC 0.037", 111G, 1979.0, P=9.219 Y  9535!;
              B 4.8M, 1.60", 76G, 1976.0; C 9.4M, 115", 51G). EA/DM.
              MIN II 3.57. B TAE AH PEE MEHEH
              CMMAPHOO  ECKA KOMOHEHTOB CCTEM AAB
              (SB 2, P=7.989268D), AC  B. BHE ATMEH HA-
              ATC CHCOAHE MEHEH ECKA CCTEM
              C A(V)=0.05M, O'CHEME CAM KOMOHEH-
              TA AB  9535! C P=0.30197D  9536!  0.30145D
               9537!. COACHO  8566!, T MEHEH HE HA-
              AC B 1970-76 ./THE RANGE OF COMBINED
              LIGHT VARIATION OF THE COMPONENTS AAB (SB 2, P=
              =7.989268D), AC, AND B IS GIVEN IN THE TABLE. OUT-
              SIDE ECLIPSES THERE ARE SINUSOIDAL LIGHT VARIATIONS
              OF THE SYSTEM WITH A(V)=0.05M DUE TO PULSATIONS OF
              THE COMPONENT AB  9535! WITH P=0.30197D  9536! OR
              0.30145D  9537!. ACCORDING TO  8566! THESE VARIATIONS
              WERE NOT OBSERVED BETWEEN 1970 AND 1976.
PI**5  ORI    MIN II 3.73. EPO TOHEH O EBM CKOPOC-
              TM./THE PERIOD IS IMPROVED USING RADIAL VELOCITIES
               4627!.
PSI    ORI    VB A (B 11.1M, 2.7", 323G; C 13.88M, 83", 196G).
              MIN II 4.58. EPO OPEEEH O EBM CKOPO-
              CTM/THE PERIOD IS DETERMINED ON THE BASE OF RADI-
              AL VELOCITIES  9541!.
R      PAV    PVAR. MAX=2411219+228.34D (J.D.2411000-18500);
              MAX=2418527+230.95D*E (J.D.2418500-30000);
              OCE/SINCE J.D.2430000-CM.TA./SEE TABLE.
S      PAV    P VAR.MAX=2421479+389.64D*E(J.D.2421000-31000);
              OCE/SINCE J.D.2431000-CM.TA./SEE TABLE. DM
              VAR CHO./STRONGLY.
              OCE MAX I HOA HAAETC MIN II./MIN II IS
              SOMETIMES OBSERVED AFTER MAX I.
T      PAV    P VAR. MAX=2413328+243.45D*E(J.D.2405700-
              25500); MAX=2425499+245.11D*E(J.D.2425500-
              32500); OCE/SINCE J.D.2432500-CM.TA./SEE
              TABLE.
V      PAV    VBA (B 14.0M VIS, 15", 327G). CPEH ECK/MEAN
              BRIGHTNESS VAR, P2=3735D, 9.7M-10.7M.
W      PAV    P VAR. O/BEFORE J.D.2431000 MAX=2413778+
              +282.92D*E; OCE/SINCE J.D.2431000-CM.TA./
              SEE TABLE.
RT     PAV    CPEH ECK/MEAN LIGHT VAR, 10.4M-11.1M  1649,
              P2=757D.
SU     PAV    P VAR. MAX=2430036+245.18D*E (J.D.2411000-30100)
               0001!; B HTEPBAE/DURING J.D.247700-40000-CM.
              TA./SEE TABLE.
SX     PAV    MU ALFA=+0.0166S, MU DELTA=-0.05".
TW     PAV    O/BEFORE J.D.2420400 MAX=2417760+397.D*E.
YY     PAV    DM VAR CHO./STRONGLY.
              BOMOHO, P CEET BOT, TOA MIN II 14.4./P
              POSSIBLY IS TWICE LONGER, IN THAT CASE MIN II 14.4.
AR     PAV    HA ATMEH/DEPTH OF ECLIPSES DM=2MB, D=
              =0.05P. PACPAC OOOKA./EXPANDING SHELL.
BD     PAV    HAAAC TOKO OHA BCKA  0629!.KTA-
               ECKA. ATMEH C EMEHTAM/ONLY ONE OUT-
              BURST WAS OBSERVED  0629!. BRIGHTNESS FLICKERING. EC-
              LIPSES ACCORDING TO THE ELEMENTS MIN I=2444412.676+
              +0.1793015D*E, DM-0.5M  9191!. BHE BCK/OUT-
              SIDE OUTBURST, 15.40M-16.21M.
BF     PAV    MIN II 11.9.
BI     PAV    MIN II (DM-0.05M) BOMOEH/IS POSSIBLE.
DF     PAV    AHA OXA MIN. OPMA KPBO ECKA CHO VAR./
              EPOCH OF MIN IS GIVEN. LINGHT CURVE SHAPE STRONGLY VAR.
DN     PAV    DS=8:.
DW     PAV    MIN II 16.3.
EG     PAV    BOMOEH BBOE OEE KOPOTK P/TWICE SHORTER P
              IS POSSIBLE  0001!.
EL     PAV    MIN II 15.5.
EN     PAV    EMEHT HATC B OTBEPEH./ELEMENTS
              NEED CONFIRMATION.
EQ     PAV    KPACHA./RED.
FY     PAV    MIN II? J.D.2436784.37.
HL     PAV    EKT AKO?/BLAZHKO EFFECT?
HP     PAV    MIN II 15.5.
HQ     PAV    MIN II 12.7.
HY     PAV    MIN II 12.1.
IL     PAV    BOMOEH T RRC./RRC TYPE IS POSSIBLE.
KR     PAV    MIN II 14.1.
KZ     PAV    VB A (B 8.7M, 6.7", 119G, 1971; C 9.2M, BC 1.0", 329G,
              1971). P VAR. MIN=2430448.617+0.949880D*E (J.D.
              2416000-30000)  0001!; OCE/SINCE J.D.2430000 -
              CM.TA./SEE TABLE. ECT MIN II./MIN II IS PRESENT.
LL     PAV    MIN II 15.1.
LO     PAV    MIN II 16.5.
LR     PAV    MIN II 15.3.
LT     PAV    MIN II 12.2.
LV     PAV    MIN II 14.3.
LY     PAV    MIN II 14.9.
MQ     PAV    AHA OXA MIN. BOMOEH T EW/KW C BBOE O-
              M P./EPOCH OF MIN IS GIVEN. EW/KW TYPE WITH
              TWICE LONGER P IS POSSIBLE.
MR     PAV    BOMOH EMEHT/POSSIBLE ELEMENTS MAX =
              =2436731.40+0.3737D*E  0001!.
MS     PAV    MIN II 14.1.
MW     PAV    D=0.08P. MIN II 8.92, DII=0.11P.
NP     PAV    OK/DEEP MIN II.
NW     PAV     A/H!=-0.7.
KAPPA  PAV    P VAR. MAX=2419619.38+9.0898D*E (J.D.2411930-
              22550); MAX=2425987.12+9.1028D*E (J.D.2422550-
              26980); MAX=2430530.67+9.0833D*E (J.D.2426980-
              31345); MAX=2433239.87+9.0956D*E (J.D.2431345-
              34045); MAX=2434693.11+9.0653D*E (J.D.2434045-
              37000); OCE/SINCE J.D.2440000-CM.TA./SEE
              TABLE.  FE/H!=0.0/-0.4. MEPEHHO BCOKA Z-KO-
              OPHATA (IZI-240 K B PEOOEH ABCMO-
              CT EPO-CBETMOCT  TA DCEP), HKA
              EBA CKOPOCT. EPO HE XAPAKTEPEH  BE
              TA CW. B CEKTPE OTMEAAC MCC CA II./MO-
              DERATELY HIGH Z COORDINATE (IZI-240 PC PROVIDED
              THE PERIOD-LUMINOSITY RELATION FOR DCEP STARS IS VA-
              LID), LOW RADIAL VELOCITY. THE PERIOD IS NOT TYPICAL
              FOR CW STARS. CA II EMISSION WAS NOTICED IN THE SPEC-
              TRUM.
LAMBDA PAV    VB A (B 12.4M, 63.1", 206G).
RO     PAV    HA OCHOBHOE KOEAHE ECKA C P1 (CM.TA.) 
              OAMTO DY=0.0069M HAKABATC KOEA-
              H/THE MAIN LIGHT VARIATION P1 (SEE TABLE) WITH A
              SEMIAMPLITUDE DY=0.0069M IS SUPERPOSED BY OSCILLA-
              TIONS WITH P2=0.1131D (DY=0.0031M), P3=0.1612D
              (DY=0.0029M).
R      PEG    OH, H2O, SIO MAEP/MASER.
              P VAR. MAX=2396327+381.9D*E (J.D.2396300-
              2408200); MAX=2413012+371.4D*E (J.D.2413000-
              19800); MAX=2420092+379.77D*E (J.D.2420000-
              31100)  0960!; OCE/SINCE J.D.2431100-CM.TA./
              SEE TABLE.
T      PEG    P VAR. MAX=2398452+371.0D*E (J.D.2398400-
              2408900); MAX=2413697+386.8D*E (J.D.2413600-
              18700); MAX=2421016+362.5D*E (J.D.2420900-
              28000)  0960!; MAX=2434343+376.0D*E (J.D.
              2428300-34300); MAX=2440984+368.7D*E (J.D.
              2434300-41000); OCE/SINCE J.D.2441000-CM.TA./
              SEE TABLE.
U      PEG    MIN II 9.73. P VAR. EMEHT COEPAT KBAPATH
              EH:/THERE IS A SQUARE TERM IN THE ELEMENTS:
              -2.468D*10**-11*E**2.0-C=0.00323D SIN  (2PI/16330)E+
              +0.418PI!. OPMA KPBO ECKA MEHETC./SHAPE OF
              THE LIGHT CURVE VARIES.
W      PEG    SIO MAEP/MASER. P VAR. MAX=2413819+343.2D*E
              (J.D.2413800-26600); MAX=2427162+345.5D*E (J.D.
              2426600-32100)  0960!; MAX=2439690+348.75D*E
              (J.D.2432300-39700)  0001!; OCE/SINCE J.D.
              2441400-CM.TA./SEE TABLE.
X      PEG    P VAR. MAX=2414713+200.3D*E (J.D.2414700-21300);
              MAX=2420105+204.3D*E (J.D.2420100-23800);
              MAX=2423570+199.8D*E (J.D.2423600-31000)  0960!;
              MAX=2432006+208D*E (J.D.2431000-32100);
              MAX=2434206+200.0D*E (J.D.2432100-39300); OC-
              E/SINCE J.D.2438400-CM.TA./SEE TABLE.
Z      PEG    P VAR. MAX=2415433+318.9D*E (J.D.2398800-
              2420550); MAX=2420207+328.0D*E (J.D.2420200-
              32000)  0960!; MAX=2432005+325.8D*E (J.D.2432000-
              37900); MAX=2437870+319D*E (J.D.2437500-40100);
              MAX=2442086+328.0D*E (J.D.2440100-43100); OC-
              E/SINCE J.D.2442100-CM.TA./SEE TABLE.
RR     PEG    P VAR. MAX=2417582+268.3D*E (J.D.2416700-17850)
               0001!; MAX=2417859+260.8D*E (J.D.2417850-
              21000)  0960!; OCE/SINCE J.D.2421000-CM.TA./
              SEE TABLE.
RS     PEG    P VAR. MAX=2415846+431.5D*E (J.D.2415800-18450);
              MAX=2418434+404.1D*E (J.D.2418400-24200);
              MAX=2424514+413.4D*E (J.D.2424500-34900)  0960!;
              MAX=2436496+403.4D*E (J.D.2435700-38600)  0001!;
              OCE/SINCE J.D.2438500-CM.TA./SEE TABLE.
RT     PEG    VB A (B 10.5M, 15.6", 291G). P VAR. MAX=2423609+
              +215.0D*E (J.D.2416000-24300); MAX=2428149+
              +216.6D*E (J.D.2424300-32100); OCE/SINCE
              J.D.2432100-CM.TA./SEE TABLE.
RU     PEG    VB A (B 12.5M, 12", 18G); SB 2 (PORB=0.3746D  9570!).
              HAATC TAKE OC ECKA C P=11.6S 
              50S./THERE ARE ALSO LIGHT OSCILLATIONS WITH P=11.6S
              AND 50S  9571!.
RV     PEG    OH MCC/EMISSION. KPBA ECKA/LIGHT CURVE
              (1907-1973) 9572!. P VAR. MAX=2428735+388.4D*E
              (J.D.2417000-32640); MAX=2430680+390.9D*E (J.D.
              2430200-38900); OCE/SINCE J.D.2438800-CM.
              TA./SEE TABLE.
RW     PEG    P VAR. MAX=2419393+208.4D*E (J.D.2412700-19400);
              MAX=2421520+213.0D*E (J.D.2419390-21550); MAX=
              =2427133+208.0D*E (J.D.2421500-27150); OCE/
              SINCE J.D.2427300-CM.TA./SEE TABLE.
RX     PEG    P2=110D:.
RY     PEG    VB B (A=RZ PEG; B 20", 252G).
RZ     PEG    VB A (B=RY PEG:20", 252G). SC 6/9-E. P VAR.
              MAX=2423361+441.4D*E (J.D.2411400-26450); MAX=
              =2431215+434.0D*E (J.D.2426400-33000); OCE/
              SINCE J.D.2433000-CM.TA./SEE TABLE.
SS     PEG    P VAR. MAX=2416390+410.8D*E (J.D.2415500-20000);
              MAX=2422235+423.8D*E (J.D.2420000-27000); MAX=
              =2427270+403.4D*E (J.D.2427000-29000); MAX=
              =2437218+416.35D*E (J.D.2428500-43000); OCE/
              SINCE J.D.2443000-CM.TA./SEE TABLE.
SV     PEG    H2O MCC/EMISSION.
SX     PEG    S 2.5/6 E. P VAR. MAX=2436043+306.56D*E (J.D.
              2414800-38300); OCE/SINCE J.D.2438300-CM.
              TA./SEE TABLE.
TU     PEG    P VAR. MAX=2417800+320.8D*E (J.D.2404300-18450);
              MAX=2420730+328.4D*E (J.D.2418450-20800);
              MAX=2428080+319.6D*E (J.D.2420800-31600); OC-
              E/SINCE J.D.2432800-CM.TA./SEE TABLE.
TW     PEG    H2O MAEP/MASER. HA OCHOBHOE MEHEHE ECKA C
              EPOOM 929.3D HAKABATC HEOE KOEA-
              H C EPOOM 94.13D./THE BASIC LIGHT VARIATION
              WITH THE PERIOD GIVEN IN THE TABLE IS SUPERIMPOSED
              BY SMALL OSCILLATIONS WITH P=94.13D.
TY     PEG    MIN II 10.2. P VAR. MIN I HEL=2419520.476+
              +3.0922754D*E (J.D.2412300-19600)  2389!; MIN I HEL=
              =2425918.348+3.092252D*E (J.D.2419600-26000)
               0001!; OCE/SINCE J.D.2426000-CM.TA./SEE
              TABLE.
TZ     PEG    P VAR? MAX=2425892+213.7D*E (J.D.2410000-28000);
              OCE/SINCE J.D.2430000-CM.TA./SEE TABLE.
UU     PEG    OH, H2O MAEP/MASER.
UW     PEG    COACHO/ACCORDING TO  8837! P=60D.
UX     PEG    P VAR. MIN=2428428.386+1.544618D*E (J.D.2422100-
              28430)  0230!; MIN=2431273.597+1.544632D*E
              (J.D.2428420-34000)  0001!; OCE/SINCE J.D.2434000-
              CM.TA./SEE TABLE.
VV     PEG    DS=8. P VAR. MAX=2420105.296+0.48837765D*E
              (J.D.2420000-28900); MAX=2433217.268+0.48838307D*E
              (J.D.2432800-38000)  3506!; OCE/SINCE
              J.D.2438000-CM.TA./SEE TABLE.
VW     PEG    P=2.341295D?
VX     PEG    HA OCHOBHOE KOEAHE ECKA HAKABAETC BTO-
              PHOE C P=80-90D:./THE BASIC LIGHT VARIATION IS
              SUPERIMPOSED BY THE SECONDARY ONE WITH P=80-90D:.
VZ     PEG     FE/H!=-1.75.
WW     PEG    P VAR. MAX=2433142+371.6D*E (J.D.2415670-33200)
               0001!; OCE/SINCE J.D.2436800-CM.TA./SEE
              TABLE.
ZZ     PEG    MIN II 12.5.
AE     PEG    P VAR. MAX=2415470.866+0.4967388D*E (J.D.2415500-
              21000); MAX=2426161.544+0.496725D*E (J.D.2425400-
              31500); MAX=2432632.809+0.496692D*E (J.D.2431500-
              36000)  0001!; B HTEPBAE/DURING J.D.2436000-
              40000-CM.TA./SEE TABLE. DS=6.3.
AG     PEG    SB 2 (PORB=820D  9580!). MAX ECKA - B 1870 ., A-
              TEM - OEH MEEHHOE AEHE ECKA, HA KOTOPOE
              C 1935 . HAKABATC EPOECKE KOEAH
              C A=0.4M V  P=PORB:/MAXIMUM OF BRIGHTNESS WAS
              IN 1870,  THEN THE VERY SLOW LIGHT DECREASE WAS OBSER-
              VED THAT WAS SUPERIMPOSED SINCE 1935 BY PERIODICAL
              LIGHT OSCILLATIONS WITH A=0.4M V AND P=PORB: MIN=
              =2428250+827D.*E (J.D.2428000-43000)  9579!.
              OCE J.D.2442300 EPO, BMO, MEHC:/ /
              AFTER J.D.2442300 THE PERIOD PROBABLY HAS CHANGED:
              MIN=2442370+760D*E  9587!.
              B 1962-1979 . ECK MEHC B PEEAX/IN
              1962-1979 THE RANGE OF BRIGHTNESS WAS 7.95M-8.55M V;
              M-M=0.50P.
              MHMM ECKA COOTBETCTBT OXAM HHEO
              COEHEH KOMOHEHTA M 3 III./LIGHT MINIMA CORRES-
              POND TO THE EPOCHS OF INFERIOR CONJUNCTION OF M 3 III
              COMPONENT.
              CEKTP/SPECTRUM VAR: BEG (1893-1919);
              C 1922.-CMOTECKA, PEM CEKTP M-BE-
               CTAHOBTC BCE OEE AMETHM./SINCE 1922 THE
              SPECTRUM IS SYMBIOTIC ONE, THE M STAR SPECTRUM BEING
              MORE NOTICEABLE.
              OKPEHA PAOTMAHHOCT AMETPOM 1" O OO-
              BHE HTEHCBHOCT EH./SURROUNDED BY A RA-
              DIO NEBULA WITH 1" HALF-POWER DIAMETER.
AN     PEG    P VAR. MAX=2428045+274.1D*E (J.D.2424500-38500)
               9581!; OCE/SINCE J.D.2438500-CM.TA./SEE
              TABLE.
AO     PEG    DS=4.3.
AQ     PEG    MIN II 10.47; D=0.030P. P VAR. MIN I=2424749.335+
              +5.548419D*E (J.D.2424000-34000)  0980!; OCE/
              SINCE J.D.2434000-CM.TA./SEE TABLE.
AT     PEG    MIN II 9.04. P VAR. MIN I=2425862.337+1.1460988D*E
              (J.D.2425800-37500)  0001!; MIN I=2437497.542+
              +1.146080D*E (J.D.2437490-40000)  6101!; MIN I=
              =2440407*4370+1.1461007D*E (J.D.2440000-42400)
               0001!; OCE/SINCE J.D.2442400-CM.TA./SEE
              TABLE.
AU     PEG    EEA B TECHO BOHO CCTEME./CEPHEID IN A
              CLOSE BINARY SYSTEM.
              SB 1 (PORB=53.319D, K1=41.8 KM/S, GAMMA=-4.1 KM/S,
              E=0.12  9582!).  FE/H!=0.1.
              P VAR. MAX=2428729.76+2.3978D*E (J.D.2426500-
              28750)  0916!; MAX=2433151.976+2.38934D*E (J.D.
              2433150-35800); MAX=2439039.08+2.39079D*E
              (J.D.2435800-39100)  0001!; OCE/SINCE J.D.
              2441700-CM.TA./SEE TABLE.
              EMEHT PBEEHHE B TAE, COEPAT KBA-
              PATH EH:/THERE IS A SQUARE TERM IN THE ELE-
              MENTS GIVEN IN THE TABLE:+2.246D*10**-6*E**2.
              OPMA KPBO ECKA MEHETC:/THE SHAPE OF THE
              LIGHT CURVE VARIES: 0.20P< M-M<0.47P.
AV     PEG    P VAR. MAX=2416347.713+0.39036510D*E (J.D.
              2414000-26500)  0752!; MAX=2426582.301+
              +0.39037015D*E (J.D.2426500-36000)  9584!; OCE/
              SINCE J.D.2436000-CM.TA./SEE TABLE.  FE/H!=
              =+0.02.
AW     PEG    D=0.07P, MIN II 7.60.
BB     PEG    HA/DEPTH OF MIN II 0.60M. EMEHT, PBEEH-
              HE B TAE, COEPAT KBAPATH EH:/THERE
              IS A SQUARE TERM IN THE ELEMENTS GIVEN IN THE TABLE:
              +2.3D*10**-11*E**2. DI=0.05P; DII=0.00P.
BF     PEG    P VAR. MAX=2426589.293+0.495796D*E+2.8D*10**-9*E**2
              (J.D.2426500-28800)  0522!; MAX=2433200.312+
              +0.495796D*E (J.D.2429400-33200)  0001!; MAX=
              =2437583.343+0.495674D*E (J.D.2437500-39400)
               0001!; OCE/SINCE J.D.2442650-CM.TA./SEE
              TABLE.
BG     PEG    P VAR. MIN=2427386.3705+1.952452D*E (J.D.2426000-
              35000)  3567!; MIN=2436453.509+1.95238D*E (J.D.
              2435000-43500)  3624!; OCE/SINCE J.D.2443500-
              CM.TA./SEE TABLE.
BH     PEG    P VAR. MAX=2426596.535+0.64101381D*E (J.D.
              2426500-28200)  1038!; OCE/SINCE J.D.2434400-
              CM.TA./SEE TABLE.
              EKT AKO/BLAZHKO EFFECT. A VAR. MAX (O-C)=
              =2442929.03+39.8D*N  9588!. (K-B)2=0.09; DS=5.
BI     PEG    HAKABATC BOH C KOM 60-80D./WAVES WITH
              A CYCLE OF 60-80D ARE SUPERIMPOSED.
BK     PEG    MIN II 10.47.
BO     PEG    MIN II 11.6. P VAR. MIN I=2427655.460+0.5804342D*E
              (J.D.2426500-35100)  2263!; OCE/SINCE J.D.
              2444000-CM.TA./SEE TABLE.
BP     PEG    P1=0.084510D; P1:P0=0.77. EPO EH/BEAT
              PERIOD PB=0.3698D  6604!.
BU     PEG    EMEHT PECTABT HAEH B HTEPBAAX/
              OBSERVATIONS ARE REPRESENTED BY THE ELEMENTS IN THE
              INTERVALS J.D.2432000-34000, J.D.2438200-41400.
BX     PEG    HA/DEPTH OF MIN II 0.62M; DI=0.05P; DII=0.00P.
              P VAR. MIN I=2431323.278+0.2804238D*E (J.D.
              2424700-39000)  0279!; OCE/SINCE J.D.2439000-
              CM.TA./SEE TABLE.
BY     PEG    P VAR. MIN I=2424745.75+0.34193403D*E (J.D.
              2424700-35400); OCE/SINCE J.D.2435000-CM.
              TA./SEE TABLE.
CC     PEG    MIN II 12.9.
CG     PEG    DS=2. P VAR?
CU     PEG    D=0.010P. P VAR. MIN=2433895.463+3.8801345D*E
              (J.D.2425500-34000)  0001!; MIN=2434221.392+
              +3.880196D*E (J.D.2434000-36500)  7929!; OCE/
              SINCE J.D.2436500-CM.TA./SEE TABLE.
CZ     PEG    MIN II 13.9.
DF     PEG    MIN II 9.2.
DG     PEG    P VAR. MAX=2425857+148.15D*E (J.D.2425500-
              33500); OCE/SINCE J.D.2433500-CM.TA./SEE
              TABLE.
DH     PEG    P VAR. MAX=2414981.537+0.25550478D*E (J.D.
              2414000-24000)  1158!; MAX=2427695.390+
              +0.2555107D*E (J.D.2424000-33500)  9590!; OCE/
              SINCE J.D.2433500-CM.TA./SEE TABLE.  FE/H!=
              =-0.9.
DI     PEG    MIN II 9.59. P VAR. MIN I=2425644.315+0.7118144D*E
              (J.D.2425500-30000)  2431!; MIN I=2437559.4096+
              +0.7118182D*E (J.D.2430000-40000)  9592!; MIN I=
              =2440159.6796+0.71181417D*E (J.D.2440000-44500);
              OCE/SINCE J.D.2444500-CM.TA./SEE TABLE.
DK     PEG    D=0.04P. P VAR. MIN=2427745.388+1.631801D*E
              (J.D.2427700-33700); OCE/SINCE J.D.2433700-
              CM.TA./SEE TABLE.
DM     PEG    D=0.03P; MIN II 11.0.
DN     PEG    CPEH ECK MEHETC C KOM 800-1400D  A=
              =0.2M-0.4M./MEAN BRIGHTNESS VARIES WITH CYCLES 800-
              1400D AND A=0.2M-0.4M.
DO     PEG    P VAR. MIN=2434272.350+2.61394D*E (J.D.2428000-
              34700)  0485!; OCE/SINCE J.D.2434700-CM.TA./
              SEE TABLE.
DV     PEG    MIN II 12.1.
DY     PEG    P VAR. MAX=2432751.9624+0.072926372D*E (J.D.
              2429000-38000); OCE/SINCE J.D.2438000-CM.
              TA./SEE TABLE.
              HA OCHOBHOE KOEAHE HAKABAETC BTOPOE C
              P1/THE BASIC PULSATION IS SUPERIMPOSED BY THE SE-
              CONDARY ONE WITH P1=0.05570D  9594!.
              A VAR, M-M VAR (=0.2358D): 0.55M< A<0.67M,
              0.24P<M-M<0.42P. DS=6.
DZ     PEG    P VAR. MAX=2429127.211+0.6073407D*E (J.D.
              2419000-28800); MAX=2429127.189+0.6073761D*E
              (J.D.2429100-33500); OCE/SINCE J.D.2433500-
              CM.TA./SEE TABLE.
EE     PEG    MIN II 7.06. TPETE TEO/THE THIRD BODY (PORB=
              =1464D, T0=2443120).
EF     PEG    VB B (A 14.0M; B 5", 305G).
EH     PEG    D=0.08P.
EQA    PEG    VB A (B=EQB PEG; A=6.87", PORB=359 YR, E=0.20.
               9597!);MU=0.560", P=91.7G. A (B)>1.4M.
EQB    PEG    VB B (A=EQA PEG). CM./SEE EQA PEG. A(U)>1.9M.
ET     PEG    DS=4.
EU     PEG    MIN II 12.3.
EZ     PEG    16 HOP 1943 .  BE HAAC CEKTP B
               2875!; BOMOHO, B TO BPEM  HEE A BC-
              KA./ON 1943 NOVEMBER 16 THE SPECTRUM OF THE STAR
              WAS B  2875!; PROBABLY AT THAT TIME THE STAR HAD A
              FLARE.
FL     PEG    MIN II 14.0.
FU     PEG    EKT AKO/BLAZHKO EFFECT (=150D); A VAR;
              15.2M<MAX<15.8M; 0.15P<M-M<0.50P.
GH     PEG    HA/DEPTH OF MIN II 0.13M.
GR     PEG    P VAR. MAX=2436492+69.93D*E (J.D.2436420-38740);
              OCE/SINCE J.D.2440470-CM.TA./SEE TABLE.
GT     PEG    MU=0.51", P=96G. AHA OXA MIN ECKA./EPOCH OF
              THE LIGHT MINIMUM IS GIVEN.
              P BCKAX A(U)<3.6M./DURING THE FLARES A(U)<
              <3.6M.
GV     PEG    DS=5:.
GW     PEG    MIN II 15.1.
GX     PEG    SB 1 (PORB=2.340939D  6103!).
GZ     PEG    VB A (B 10.6M, A3V, 32.7", 198G).
HN     PEG     FE/H!=-0.09. AHA OXA MIN ECKA./EPOCH OF
              LIGHT MINIMUM IS GIVEN.
              OTMEEHA EPEMEHHOCT MCC B HX H 
              K CALL C P=4.63D/THE VARIABILITY OF EMISSION IN H
              AND K CALL LINES WITH P=4.63D WAS DETECTED  9600!.
HP     PEG    VR=-381 KM/S.
HR     PEG    S4+/1+.
HZ     PEG    MIN II 17.6.
II     PEG    MU=0.575", P=86.5G. SB 1 (TO=2443030.396+6.724464D*E);
              T0-OXA HHEO COEHEH K-BE./T0 IS
              THE EPOCH OF THE INFERIOR CONJUNCTION OF K-STAR.
              B TAE PBEEHA OXA MAX CTOPCOHHO BO-
              H. CPEH ECK CCTEM MEHETC./THE EPOCH
              OF THE DISTORTION WAVE MAXIMUM IS GIVEN IN THE TABLE.
              MEAN BRIGHTNESS OF THE SYSTEM VARIES.
IK     PEG    SB 1 (PORB=21.724D). MTEPOHOCT/MULTIPE-
              RIODICITY  9609!.
IM     PEG    SB 1 (PORB=24.649D).
BETA   PEG    VB A (B 11.2M, 109", 211G).
EPSILO PEG    VB A (B 12.66M, 81", 325G; C 8.65M, 140", 321G). O-
              HO VAR B PEEAX 2.29M-2.44M V. 26/27 CEHTP
              1972. B HTEPBAE 23H58M-00H02M UT A PKA
              (0.7M V), ATEM, K 00H09M UT OCAA O 2.4M V
               6875!. 5 HOP 1847. A 3.5M, ATEM CTAA
              PE, HO 6 HOP ECK BE BCE EE OCTABAC
              CAEE HOPMAHOO  9606!./USUALLY VARIES IN THE
              RANGE 2.29M-2.44M V. ON 1972 SEPTEMBER 26/27 IN THE
              INTERVAL 23H58M-00H02M UT IT WAS BRIGHT (0.7M V),
              THEN AT 00H09M UT DECREASED TO 2.4M V  6875!. ON
              1847 NOVEMBER 5 THE STAR WAS 3.5M, THEN THE BRIGHT-
              NESS INCREASED BUT ON NOVEMBER 6 IT WAS STILL FAINTER
              THAN NORMAL  9606!.
TAU    PEG    P2=0.04895D; PB=0.4943D.
S      PER    CM./SEE SU PER. OH, H2O, SIO MAEP/MASER.
              B 1920-1969-BTOPHE BOH C KAM 300D-
              700D  DM-1M  8630!; B 1935-1961 P1=807D, P2=
              =930D  9694!./IN 1920-1969 THERE WERE SECONDARY
              WAVES WITH CYCLES OF 300D-700D AND DM-1M  8630!;
              IN 1935-1961 P1=807D, P2=930D  9694!.
T      PER    OTMEAC PE EPOHOCT./OTHER PERIODI-
              CITIES WERE NOTED. CM./SEE SU PER.
U      PER    P VAR. MAX=2411683+316.10D*E (O/BEFORE J.D.
              2422500); MAX=2422748+326.53D*E (J.D.2422500-
              34000); OCE/SINCE J.D.2434000-CM.TA./SEE
              TABLE.
V      PER    VB A (B 14M, 28", 278G).
W      PER    P2=2667D+-460D HAKABAETC/IS SUPERIMPOSED.
X      PER    3U 0352+30. LX/LOPT=10**-2. ADS 2859 A (B=
              =V397 PER, M3III, 22.5", 12G). SB. K-TOK.
              PEHTEHOBCK CAP/IR EXCESS. X-RAY PULSAR
              (P=13.93M).
              B PEHTEHOBCKX, OTECKX, CEKTPAHX HA-
              EHX OTMEAC TAKE EPOHOCT:/FURTHER
              PERIODICITIES WERE NOTICED IN X-RAY, OPTICAL, SPECTRO-
              SCOPIC OBSERVATIONS: 22.4H, 308.33D, 580.7D.
Y      PER    P VAR. MAX=2414990+254.74D*E (J.D.2415000-18000);
              MAX=2418049+246.25D*E (J.D.2418000-22000);
              MAX=2422242+253.62D*E (J.D.2422000-41000);
              OCE/SINCE J.D.2441000-CM.TA./SEE TABLE.
Z      PER    D=0.028P; MIN II 9.8.
              P VAR. MIN=2418173.663+3.056422D*E (J.D.2415000-
              19000)  1961!; MIN=2425481.416+3.05636D*E
              (J.D.2419000-31000)  0978!; OCE/SINCE J.D.
              2431000-CM.TA./SEE TABLE.
RR     PER    P VAR.MAX=2424280+392.01D*E (J.D.2416000-28500);
              OCE/SINCE J.D.2428500-CM.TA./SEE TABLE.
RS     PER    CM./SEE SU PER. COACHO/ACCORDING TO  1053!, P=
              =152D.
RT     PER    MIN II 10.67. P VAR. MIN=2411963.2995+0.84941322D*E
              (J.D.2411317-19400); MIN=2419702.3124+
              +0.84940248D*E (J.D.2419400-29300); MIN=
              =2429751.6066+0.84941274D*E (J.D.2429300-33000);
              OCE/SINCE J.D.2433000-CM.TA./SEE TABLE.
RV     PER    MIN II 10.4. P VAR. MIN=2417972.345+1.973489D*E
              (J.D.2417000-25500); OCE/SINCE J.D.2432500-
              CM.TA./SEE TABLE.
RW     PER    OPMA KPBO ECKA/THE LIGHT CURVE SHAPE VAR,
              D=0.03P-0.000P. MIN II 9.78. P VAR. O/BEFORE J.D.
              2425720 MIN=2425720.0185+13.198910D*E;
              MIN=2429217.5946+13.198399D*E (J.D.2425720-
              36700); OCE/SINCE J.D.2436700-CM.TA./SEE
              TABLE.
RY     PER    D=0.014P; MIN II 8.65.
RZ     PER    S 3/7 E. P VAR. O/BEFORE J.D.2430500 MAX=2415034+
              +353.19D*E; OCE/SINCE J.D.2430500-CM.TA./
              SEE TABLE.
ST     PER    VB A (B 12.1M, 11.6", 6G, 1928). D=0.014P, MIN II 9.62.
              P VAR. MIN=2419030.5038+2.6483615D*E
              (J.D.2418500-27000)  9740!; MIN=2429528.5897+
              +2.6483488D*E (J.D.2427000-34600)  2389!; MIN=
              =2439091.716+2.648353D*E (J.D.2439000-42400);
              OCE/SINCE J.D.2442400-CM.TA./SEE TABLE.
SU     PER    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER H, HI PER.
SV     PER     A/H!=0.6. SB 2, OP CTHK/HOT COMPANION.
              P VAR? O/BEFORE J.D.2435000 MAX=2419055.145+
              +11.12875D*E  2431!; OCE/SINCE J.D.2435000-
              CM.TA./SEE TABLE.
SX     PER     A/H!=0. KAPTA B  8300! HEBEPHA./THE CHART IN
               8300! IS WRONG.
SY     PER    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 1528.
TU     PER    DM, P VAR. O/BEFORE J.D.2427200 MAX=2418572.288+
              +0.6070775D*E; MAX=2427119.334+0.6070643D*E
              (J.D.2427200-36000); OCE/SINCE J.D.2436000-
              CM.TA./SEE TABLE.
TV     PER    P2=1080D HAKABAETC/IS SUPERIMPOSED.
TX     PER     FE/H!=-0.88. OH MAEP/MASER.
TZ     PER    VB A (B14M, 13", 290G). MU ALFA=+0.012", MU DELTA=-0.050".
              CM./SEE SU PER.
UX     PER     A/H!=-0.3.
UY     PER     A/H!=-0.3. B PAOHE PACCEHHX CKOEH/IN
              THE REGION OF THE OPEN CLUSTERS KING 4, CZERNIK 8.
UZ     PER    P2=91D HAKABAETC/IS SUPERIMPOSED.
VV     PER    BOMOEH BBOE OEE KOPOTK P/TWICE SHORTER
              P IS POSSIBLE  0960!.
VX     PER    CM./SEE SU PER.  A/H!=-0.2. P VAR. OCE/SINCE
              J.D.2431000-CM.TA./SEE TABLE.
VY     PER    CM./SEE SU PER.  A/H!=-0.3.
VZ     PER    VB A (B 16.9M PG, 17", 180G). CM./SEE DY PER.
WY     PER    P VAR. MIN=2425234.460+3.327126D*E (J.D.2421500-
              26000)  1072!; OCE/SINCE J.D.2441500-CM.TA./
              SEE TABLE.
XX     PER    VB A (B 9.7M VIS, 21", 176G, 1909).
              CPEH BEHA/MEAN BRIGHTNESS VAR, P=4100D.
XY     PER    ADS 2788 AB (DMV=0.6M-2.5M, 1.4", 75G, SPA=A2II,
              SPB=B6E). K TOK./IR EXCESS.
XZ     PER    MIN II 11.6. P VAR? MIN=2425150.439+1.1516282D*E
              (J.D.2425000-29000)  0522!; MIN=2437932.411+
              +1.1516347D*E+0.005D SIN (0.09091G*E) (J.D.2432000-
              38000)  0001!; OCE/SINCE J.D.2438000-CM.TA./
              SEE TABLE.
YZ     PER    CM./SEE SU PER.
ZZ     PER    KOOPHAT, BOMOHO, HEBEPH./THE COORDINATES
              ARE POSSIBLY ERRONEOUS.
AB     PER    D=0.045P; MIN II 10.5. VB (DM=0.0M VIS, 0.20", 86.4G,
              1978).
AD     PER    CPEH ECK/MEAN BRIGHTNESS VAR, P=2950D.
              CM./SEE SU PER.
AE     PER    P2=2150D HAKABAETC./IS SUPERIMPOSED.
AG     PER    ADS 2990 A (B DM=2.0M, 0.9", 225G, 1975; C 12.6M,
              36", 118G, 1948). AH CMMAPH ECK AB./THE COM-
              BINED BRIGHTNESS AB IS GIVEN. MIN II 7.00, DII=0.10P,
              DII=0. BPAEHE H AC/APSIDAL MOTION:
              MIN II-MIN I=1.01435D+0.0884D SIN (0.0278G*E+
              +49.1G).
AR     PER    P VAR, KBAPATH EH/NONLINEAR TERM:+1.18D*
              *10**-11*E**2.  FE/H!=-0.17.
AS     PER    DM VAR, D (DB)/DT=-0.01M/YR.
AV     PER    P=250-300D.
AW     PER    SB 2, CTHK/COMPANION B6V, DM (COMPANION-AW)=
              =2.8M VIS.
AX     PER    AHA OXA MIN. EPEMEHHOCT C DM O 0.7M PG, BE-
              POTHO, CBAHA C OPTAHM BEHEM. HA-
              AETC BCEHA AKTBHOCT./EPOCH OF MIN
              IS GIVEN. THE VARIABILITY WITH DM UP TO 0.7M PG IS
              CAUSED PROBABLY BY THE ORBITAL MOTION. OUTBURST AC-
              TIVITY IS SUPERIMPOSED.
AY     PER    D=0.009P.
BE     PER    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER CR 39.
BI     PER    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER BERK 9.
BL     PER    P=125-130D.
BM     PER     FE/H!=-0.04.
BP     PER    MIN II=MIN I. CM./SEE BE PER.
BU     PER    ECK B MAX MEHETC/MAX BRIGHTNESS VAR, P=8.1YR
               1085!. CM./SEE SU PER.
CC     PER    MIN II 14.1.
CI     PER    P VAR (3.35D-3.40D), BOMOHO, C EPOOM/POSSIBLY
              WITH A PERIOD OF 4000D. OPMA KPBO ECKA/THE
              LIGHT CURVE SHAPE VAR.
CK     PER    D=0.05P:.
CM     PER    D=0.052P. CM./SEE CO PER.
CO     PER    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER STOCK 2.
CR     PER    EMEHT TPET OTBEPEH./ELEMENTS NEED
              CONFIRMATION. CM./SEE CO PER.
CS     PER    CM./SEE CO PER.
CZ     PER    CM./SEE SU PER.
DE     PER    D=0.01P?
DF     PER    CM./SEE SU PER.
DG     PER    D=0.021P.
DK     PER    HA/THE DEPTH OF MIN II 0.05M. CM./SEE SU PER.
DM     PER    MIN II 8.02, DII=0.17P. H MHMMOB, OPMA
              MIN II VAR./DEPTHS OF MINIMA, THE SHAPE OF MIN II VAR.
              CM./SEE SU PER.
DO_DP  PER    CM./SEE SU PER.
DR_DU  PER    CM./SEE SU PER.
DV     PER    MIN II 14.5.
DY     PER    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER TR 2.
DZ     PER    MIN II 14.7. CM./SEE DY PER.
EL     PER    O/BEFORE J.D.2428900 MAX=2427980+167D*E;
              B HTEPBAE/DURING J.D.2428900-31000-CM.TA./
              SEE TABLE.
EO     PER    K TOK?/IR EXCESS?
ER     PER    CPEH ECK/MEAN BRIGHTNESS VAR, P-900D.
EU     PER    CM./SEE ER PER.
EW     PER    HAKABATC BOH/SUPERIMPOSED WAVES 70D-180D.
              CM./SEE HS PER.
EX     PER    MIN II 12.5.
FM     PER    VB A (B 12.1M, 3", 285G). P VAR? MAX=2429982.268+
              +0.489199D*E (J.D.2428000-30600); B HTEPBAE/
              DURING J.D.2433700-36000-CM.TA./SEE TABLE.
FR     PER    CM./SEE SY PER.
FV     PER    K/CYCLES 300-350D, 1800D:.
FX     PER    D=0.04P. B OACT PACCEHHOO CKOEH/IN THE
              REGION OF THE OPEN CLUSTER NGC 1582.
FY     PER    BOMOHE EPO/POSSIBLE PERIODS 0.0702D,
              0.4407D. OTOMETPECK CEKTPAH KACC/
              PHOTOMETRIC SPECTRAL TYPE B1V.
FZ     PER    CM./SEE SU PER.
GH     PER    P=220D BOMOEH/IS POSSIBLE.
GK     PER    SB 2 (SDBE+K2IVP).
              OCE BOBPATA K OBCEHOM ECK OKABA-
              ET CEE B AKTBHOCT: CTPE HEPAB-
              HE MEHEH (DM-0.1M A HECKOKO MHT ; HE-
              PABHE KTA OT CTOK K CTKAM (DM O
              0.3M); MEEHHE HEPABHE KOEAH (DM=
              =1.5M A HECKOKO ECTKOB CTOK); BCK C
              BOPACTAHEM ECKA A 10D-30D  CAOM A 10D-
              40D, DM O 3.5M, CPEH HTEPBA ME BC-
              KAM DT=820D  9686, 9788!. COACHO  10198!,
              EBE CKOPOCT PECTABTC EMEHTAM
              MAX (VR>0)=2444912.966+1.996803D*E (KABS=
              =124 KM/C, KEM=34 KM/C. COACHO  10199!, 2D-
              KOEAHE MOPOBAHO EPOOM 0.131623D,
              MAX (DVR>0)-2443787.995 (KABS=15 KM/C, KEM=
              =20 KM/C). BO BPEM BCK APECTPPOBAHA
              CHCOAHA MO PEHTEHOBCKOO OTOKA,
              TMAX=2445555.67456+0.004066443D*E  9786!.
              PACPAC OOOKA (0.454"/O, 1948-1964;
              0.432"/O, 1964-1981,   9787!)./THE FOLLOWING TY-
              PES OF ACTIVITY ARE BEING OBSERVED AFTER THE RETURN
              TO THE NORMAL BRIGHTNESS: RAPID IRREGULAR VARIATIONS
              (DM-0.1M IN SEVERAL MINUTES); IRREGULAR FLUCTUATIONS
              FROM NIGHT TO NIGHT (DM UP TO 0.3M); SLOW IRREGULAR
              VARIATIONS (DM=1.5M IN SEVERAL DOZEN DAYS); BURSTS
              WITH LIGHT INCREASE IN 10D-30D AND DECREASE IN
              10D-40D, DM UP TO 3.5M, THE MEAN INTERVAL BETWEEN
              BURSTS BEING DT=820D  9686, 9788!. ACCORDING TO
               10198!, THE RADIAL VELOCITIES ARE REPRESENTED WITH
              THE ELEMENTS MAX (VR>0)=2444912.966+1.996803D*E
              (KABS=124 KM/S, KEM=34 KM/S). ACCORDING TO
               10199!, THE 2D VARIATION IS MODULATED WITH A PERIOD
              OF 0.131623D, MAX (DVR>0)-2443787.995 (KABS=
              =15 KM/S, KEM=20 KM/S). DURING A BURST THE SINU-
              SOIDAL MODULATION OF X_RAY FLUX WAS RECORDED,
              TMAX=24455555.67456+0.004066443D*E  9786!.
              EXPANDING ENVELOPE (0.454"/YR, 1948-1964;
              0.432"/YR, 1964-1981,  9787!).
GP     PER     A/H!=-0.5.
GQ     PER    COACHO/ACCORDING TO  0021!, SP KO.
HQ     PER     A/H!=-0.3.
HS     PER    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER STOCK 4.
HV     PER    D-0.03P.
HW     PER    MIN II 13.3. MIN II-MIN I=0.45P:.
HY     PER    TP  ETPEX MIN   1079! EMEHTAM HE PE-
              CTABTC./THREE OF THE FOUR MIN IN  1079! ARE NOT
              SATISFIED WITH THE ELEMENTS.
HZ     PER     A/H!=-0.8. B_V:+1.93, +2.34.
II     PER    MIN II 13.6. B OACT PACCEHHOO CKOEH/IN
              THE REGION OF THE OPEN CLUSTER NGC 1582.
IK     PER    MIN II 11.6.
IM     PER    MIN II 12.7. EMEHT HATC B OTBEPEH./
              THE ELEMENTS NEED CONFIRMATION. CM./SEE BE PER.
IO     PER    H2O MAEP/MASER.
IP     PER    K TOK./IR EXCESS.
IQ     PER    DI=0.02P. MIN II 7.88, DII=0.12P, DII=0.03P, MIN II-
              -MIN I=0.53P. P VAR? VB A (B=BD+47G921, 9.30M,
              A0V P:, 39.3", 175G); SB 1.
IT     PER    DI=0.06P. MIN II 10.0, DII=0.24P:, DII=0.16P:.
              VB (DM=1.7M, 12", 37G). AH PEE MEHEH
              CMMAPHOO ECKA./THE RANGE OF THE COMBINED
              BRIGHTNESS IS GIVEN.
IW     PER    SB 1. MIN II 5.83.
IX     PER    HA/THE DEPTH OF MIN II 0.02M.
              VB A (B 10.6M, 5", 208G).
IZ     PER    MIN II 8.3.
KK     PER    CM./SEE SU PER.
KP     PER    EH:/BEAT PHENOMENON:P1-CM.TA./SEE TABLE,
              A1=0.0323M B; P2=0.1980855D, A2=0.0235M B; P3=
              =0.2270986D, A3=0.0072M B.
KR     PER    MIN II 11.1.
KS     PER    SB (PORB=360.47D). ABH KOMOHEHT-EEBA
              BEA. OMMO OPABHO EPEMEHHOCT (CM.
              TA.), OTMEAC KOEAH C P=50-100 MH 
              DM B HECKOKO COTX BEHO BEH. K -
              TOK. EPEMEHHA OPA (P-1%)./THE MAIN
              COMPONENT IS A HELIUM STAR. BESIDES THE SEMIREGULAR
              VARIABILITY (SEE TABLE),  VARIATIONS WERE NOTED WITH
              P=50-100 MIN AND DM OF SEVERAL HUNDREDTHS OF A
              MAGNITUDE. IR EXCESS. VARIABLE POLARIZATION (P-1%).
KT     PER    KBAEPOECKE KOEAH BO BPEM BCEK:/
              QUASI-PERIODIC OSCILLATIONS DURING OUTBURSTS: P=
              =22.9S-29.5S  5959!, 82S, 90S, 147S  9791!, DM O/
              UP TO-0.01M.
KV     PER     FE/H!=-0.96. P VAR. MAX=2428950.400+0.24942D*E
              (J.D.2428950-29200); OCE/SINCE J.D.2429500-CM.
              TA./SEE TABLE.
KW     PER    MIN II 10.8. P VAR. MIN=2426295.450+0.931255D*E
              (J.D.2423400-39500)  4009!; OCE/SINCE J.D.
              2440000-CM.TA./SEE TABLE.
KY_LQ  PER    CM./SEE SU PER.
LR     PER    OEH KPACHA./VERY RED. CM./SEE SU PER.
LX     PER    MU ALFA=+0.0065S, MU DELTA=-0.063". MIN II 8.38M.         .
DII=0.05P
              MPPA BOHA:/MIGRATING DISTORTION WAVE:
              P=475D  9792!, DM O/UP TO 0.04M.
MS     PER    MIN II 12.1.
MX     PER    K TOK./IR EXCESS.
NP     PER    MIN II 13.0.
NR     PER    P VAR. MAX=2416780+323.0D*E (J.D.2415750-
              24550); MAX=2435060+340.2D*E (J.D.243350-35400);
              OCE/SINCE J.D.2436700-CM.TA./SEE TABLE.
NU     PER    TECHA APA, VAR-HA BEA./A CLOSE PAIR, VAR
              IS THE SOUTHERN STAR.
OV     PER    D-2H.
PP     PER    CM./SEE SU PER.
PR     PER    CM./SEE SU PER.
QR     PER    KPACHA./RED.
QU     PER    D=0.03P.
QW     PER    MIN II 14.7:.
QX     PER    MIN II 16.1.
V345_  V347   PER B TMAHHOCT/IN THE NEBULA NGC 1579.
V351_  V352   PER CM./SEE SU PER.
V354_  V356   PER CM./SEE SU PER.
V357   PER    CM./SEE SUPER. P=0.21955D BOMOEH/IS POSSIBLE.
V358_  V359   PER CM./SEE SU PER.
V360   PER    CM./SEE SU PER. PE BOMOHE EPO:/
              OTHER POSSIBLE PERIODS: 0.40036D, 0.40154D.
V361   PER    CM./SEE SU PER.
V363   PER    KPACHA./RED.
V364   PER    MIN II 15.6, MAX II 14.8.
V365   PER    MIN II 14.3:.
V376   PER    P2=0.09165D, A2=0.016M;P1-CM.TA./SEE TABLE,
              A1=0.037M. A VAR.
V380   PER    SB (PORB=26D?). AHA OXA MIN ECKA./THE EPOCH
              OF MIN LIGHT IS GIVEN.
V382   PER    CM./SEE SU PER.
V392   PER    H KOMOHEHT OEH TECHO AP./THE SOUTHERN
              COMPONENT OF A VERY CLOSE PAIR.
V394   PER    H2O MAEP/MASER.
V395   PER    VB A (B 3.5", 90G).
V396   PER    B OACT PACCEHHOO BEHOO CKOEH/IN THE
              REGION OF THE OPEN CLUSTER ALFA PER.
              HAEHM OBETBOPET TAKE/OBSERVATIONS
              ARE ALSO SATISFIED BY P-1.678D. COACHO/ACCORDING
              TO  7586!, P=2.4928D /OR 1.6857D.
V397   PER    ADS 2859 B (A=X PER; B 22.5", 12G).
V398   PER    BOMOEH TAKE T IN./IN TYPE IS ALSO POSSIBLE.
V403   PER    CM./SEE SU PER.
V409   PER    AHA OXA MIN./EPOCH OF MIN IS GIVEN.
V423   PER    ADS 2433 A (B 11.9M, 30.8", 99.2G); SB.
              AH PORB./PORB IS GIVEN.
V424   PER    CM./SEE SU PER. K TOK./IR EXCESS.
V425   PER    VB A (B 12.8M, 3.6"; C 14.3M, 6.8"). CM./SEE SU PER.
V428   PER    COACHO/ACCORDING TO  8639!, T/TYPE IS?
V432   PER    MIN II 11.6.
V434   PER    MIN II 14.9.
V436   PER    MIN II 5.74; MIN II-MIN I=0.413P; DII=0.03P.
V437   PER    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 744.
V438   PER    CM./SEE SU PER. VB (8.7M, 10.9M, 1.2", 26G).
              MIN II 8.34. AH PEE MEHEH CMMAPHOO
              ECKA. EPEMEHHM CTAETC PK KOMOHEHT.
              TO PEOOEHE TPEET POBEPK./THE RANGE
              OF COMBINED BRIGHTNESS VARIATION IS GIVEN. THE BRIGHT
              COMPONENT IS CONSIDERED TO BE VARIABLE. THIS SUGGES-
              TION NEEDS VERIFICATION.
V439   PER    CM./SEE SU PER.
V440   PER    CM./SEE SU PER. ADS 1820 A (B 14.5M, 8.3", 122G).
V449   PER    MIN II 13.3.
V451   PER    MIN II 15.8.
V459   PER    B CKOEH ALFA PER./IN THE ALFA PER CLUSTER.
V461   PER    CM./SEE V459 PER.
V462   PER    MIN II 14.0.
V465   PER    P2=0.030D HAKABAETC/IS SUPERIMPOSED.
V466   PER    HAOEHE/SUPERPOSITION OF P1=5300D+-250D, P2=
              =475D+-35D (DM=1.1M), P3=0.26D (DM=0.5M).
V468   PER    P1=925S, P2=1022S. MU=0.29", P=170G.
V469   PER    MEHEH POE H C EPOAM/CHANGES
              OF LINE PROFILES WITH PERIODS 0.150D, 0.188D, 0.304D,
              0.476D, 0.608D, 1.88D  9814!.
              B 1978/1979 HAAC HEPAAHE CA:/
              IN 1978/1979 NON-RADIAL PULSATIONS WERE OBSERVED:
              P1=1.74D. P2=2.04D  4173, 4180!.
V470   PER    VB A (B 18.8M B, 1"-2").
V471   PER    EHTPAHA BEA AHETAPHO TMAHHOCT/THE
              CENTRAL STAR OF THE PLANETARY NEBULA M 1-2=VV8.
              COACHO/ACCORDING TO  9815, 9816!, CONST.
BETA   PER    KPATHA CCTEMA/MULTIPLE SYSTEM (ATMEHHA APA/
              ECLIPSING PAIR=ALGOL AB; ALGOL C 4.7M, AM, A=0.10",
              PORB=1.862A); ALGOL AB=ADS 2362 A (B 12.7M, 57.5",
              156G, 1920). P VAR. P=2.8673442D (1784-1835);
              P=2.8673012D (1835-1854); P=2.8672775D (1854-
              1901); P=2.8672967D (1901-1913); P=2.8672506D
              (1913-1915)  6156!; MIN I=2424477.806+2.86730236D*E
              (J.D.2420500-25000); MIN I=2425917.203+
              +2.86732697D*E (J.D.2425000-27700); MIN I=
              =2433194.454+2.86731667D*E (J.D.2427700-33600);
              MIN I=2433928.4944+2.86732442D*E (J.D.2433600-
              37000); MIN I=2437598.6766+2.86733732D*E (J.D.
              2437000-42200); OCE/SINCE J.D.2442200-CM.
              TA./SEE TABLE. B HEPABEHCTBAX POCEBAETC
              PORB (ALGOL C)=1.862A; BOMOHO, PEAEH TAKE E-
              PO 32A./PORB (ALGOL C)=1.862A MAY BE TRACED IN
              THE DEVIATIONS; A PERIOD OF 32A MAY ALSO BE REAL.
              HA/DEPTH OF MIN I VAR.
              EPEMEHHA OPA, MEHEH PO BOO-
              POHX H, BPEMEHAM MCC B CEKTPE. PAO-
              CTOHK C ACTM BCKAM PAHO AMT,
              CA PEHTEHOBCK CTOHK./VARIABLE POLARIZA-
              TION, CHANGES IN HYDROGEN LINE PROFILES, SOMETIMES
              EMISSIONS IN THE SPECTRUM. RADIO SOURCE WITH FREQUENT
              BURSTS OF DIFFERENT AMPLITUDE, FAINT X_RAY SOURCE.
DELTA  PER    EPEMEHHA MCC/VARIABLE EMISSION LAMBDA 1650 A
               6905!. VR VAR, A=16 KM/S.
KSI    PER    B AHE K OACT CEKTPA (LAMBDA=10 MU M) DM>1M;
              EPEMEHHOCT CBBAETC C OTEPE MACC./IN THE
              FAR IR RANGE (LAMBDA=10 MU M) DM>1M; THE VARIABILITY IS RE-
              LATED TO MASS LOSS.
OMIKRO PER    VB A (B 8.4M, 0.96", 29.7G, 1972). B OACT PACCEH-
              HOO CKOEH/IN THE REGION OF THE OPEN CLUSTER
              IC 348. BOMOHO HAOEHE KOEAH TA BCEP./
              POSSIBLE SUPERPOSITION OF BCEP TYPE OSCILLATIONS.
RO     PER    BOMOHO OEE MEEHHOE KOEAHE CPEHEO
              ECKA./A SLOWER VARIATION OF THE MEAN LIGHT IS POSSI-
              BLE. MU ALFA=0.0111S, MU DELTA=-0.102".
PSI    PER    SB 2 (PORB=126.696D). V SINI=450 KM/S. A VAR
              (P=PORB).
B      PER    SB 2. PAE H MIN 0.03M./DEPTHS OF MINIMA
              DIFFER BY 0.03M. TPETE TEO?/THIRD BODY?, P=701D.
              PAOCTOHK./RADIO SOURCE. B OACT PACCEHHO-
              O CKOEH/IN THE REGION OF THE OPEN CLUSTER
              NGC 1545.
R      PHE    P VAR. MAX=2405121+271.0D*E (J.D.2405000-11500);
              MAX=2414570+266.26D*E (J.D.2414500-25500);
              OCE/SINCE J.D.2425500-CM.TA./SEE TABLE.
T      PHE    P VAR. MAX=2411252+281.00D*E (J.D.2410000-30000);
              OCE/SINCE J.D.2430000-CM.TA./SEE TABLE.
W      PHE    P VAR. MAX=2414960+328.65D*E (J.D.2414500-19500);
              MAX=2424530+332.87D*E (J.D.2424500-30200);
              OCE/SINCE J.D.2436000-CM.TA./SEE TABLE.
RS     PHE    P VAR?
RT     PHE    P=208D?
RV     PHE    P VAR?; (K-B)2=0.06; DS=8:.
SX     PHE    MU=0.894", P=163.1G. P VAR. MAX=2433923.9618+
              +0.054964519D*E1-0.00337D SIN 2PI (0.28503379*E1+
              +0.074) (J.D.2433900-36900); OCE/SINCE
              J.D.2436900-CM.TA./SEE TABLE.
              EMEHT, PBEEHHE B TAE, COEPAT CH-
              COAH EH:/THERE IS A PERIODIC TERM IN THE
              ELEMENTS GIVEN IN THE TABLE:
              -0.00325D SIN 2PI (0.28503575*E2-0.107).
              COACHO  9614!  OX 1950.0/ACCORDING TO
               9614! FOR EPOCH 1950.0 P0=0.054964509D, P1=
              =0.042772831D, PB=0.1928355D; DP0/DT=-87.10**-13,
              DP1/DT=-174.10**-13, DPB/DT=-2.46*10**-10.
              P1/P0=0.778; 0.8M<A<0.3M; 0.2P<M-M<0.4P.  FE/H!=
              =-0.6.
WW     PHE    MIN II 12.7.
YZ     PHE    MIN II 13.0.
AD     PHE    MIN II 10.80. P VAR. MIN I=2436847.375+0.3799277D*E
              (J.D.2428650-36850); OCE/SINCE J.D.2436850-CM.
              TA./SEE TABLE.
AE     PHE    MIN II 8.19; 0.033P<DI<0.05P; DII=0.00P. OPMA KPBO
              ECKA MEHETC C EPOAM 55.9D  95.3D/THE SHA-
              PE OF THE LIGHT CURVE VARIES WITH PERIODS 55.9D AND 95.3D
               9615!. P VAR. MIN I=2440857.8140+0.36237459D*E
              (J.D.2438250-40870)  7388!; MIN I=2441969.57074+
              +0.36237186D*E (J.D.2440870-42000)  9616!; MIN I=
              =2442654.8201+0.3623741D*E (J.D.2441950-42660)
               9533!; OCE/SINCE J.D.2443700-CM.TA./SEE
              TABLE.
AG     PHE    MIN II 8.95. P VAR. MIN I=2440415.231+0.7553429D*E
              (J.D.2438300-40850); OCE/SINCE J.D.2443750-
              CM.TA./SEE TABLE.
AI     PHE    MIN II 8.89; DI=0.0035P; MIN II-MIN I=0.46P.
AU     PHE    MIN II 13.0. COACHO  9517!, P, AHH B TAE,
              HEBEPEH./ACCORDING TO  9517!, THE P VALUE GIVEN IN
              THE TABLE IS WRONG.
AX     PHE    MU=0.234", P=70G. MTEPOECKA:/MULTIPERIO-
              DICAL: PI=606.8S, 682.7S, 744.7S, 840.2S (AI=0.01M).
GAMMA  PHE    SB1 (PORB=193.85D).
DZETA  PHE    VB A (B 7.0M, A7:, 0.46", 51.4G, 1965.9; C 8.0M,
              F7V, 6.4"). B TAE PBEEH PEE MEHE-
              H CMMAPHOO ECKA KOMOHEHTOB A  B./TOTAL
              LIGHT RANGE OF A AND B COMPONENTS IS GIVEN IN THE
              TABLE. MIN II 4.22, MIN II-MIN I=0.507P; DII=0.02P.
IOTA   PHE    VB A (B 12.7M, 7.7", 270G).
KSI    PHE    VB A (B 12.1M, 13.2", 253G). AHA OXA MIN I (V)/
              EPOCH OF MIN I (V) IS GIVEN IN THE TABLE. A(V)=0.13M.
RO     PHE    PETAT ACTOTHOO AHAA CM. TAKE B PAO-
              TAX/FREQUENCY ANALYSIS RESULTS SEE ALSO IN  9619,
              9620, 9621!.
PSI    PHE    SB.
R      PIC    P VAR. MAX=2413413+165.8D*E (J.D.2413000-23600);
              OCE/SINCE J.D.2423600-CM.TA./SEE TABLE.
              PAK KPBO ECKA/LIGHT CURVE (1923-1953)
               1054!.
S      PIC    P VAR. MAX=2413595+424.7D*E (J.D.2405500-23000);
              OCE/SINCE J.D.2423000-CM.TA./SEE TABLE.
              OH MCC/EMISSION.
U      PIC    P VAR. MAX=2428103.565+0.44036450D*E
              (J.D.2414000-29000)  0353!; OCE/SINCE J.D.
              2438400-CM.TA./SEE TABLE. (K-B)2=0.17; DS=3.
X      PIC    MIN II 10.8.
RR     PIC    B 1965. OHAPEH EPOECKE MEHEH
              ECKA C A(B)=0.33M C EMEHTAM MAX=2438815.380+
              +0.14502545D*E. HA T KOEAH HAKABATC
              PE C A(B)=0.036M  EPOOM-15.6 MH. 
              -15.4 MH.  9612!, A TAKE CTPE OC C
              EPOAM 20-40S  9613!./SINCE 1965 PERIODIC LIGHT
              VARIATIONS WERE DETECTED WITH A(B)=0.33M AND ELE-
              MENTS MAX=2438815.380+0.14502545D*E. THESE VA-
              RIATIONS ARE SUPERIMPOSED BY OTHERS WITH A(B)=0.036M
              AND PERIOD-15.6 MIN OR-15.4 MIN  9612!. THERE ARE
              ALSO RAPID OSCILLATIONS WITH PERIODS IN THE RANGE 20-
              40S  9613!.
RT     PIC    HE BHA  HA OHO ACTHKE; BOMOHO, E-
              EKT./NOT SEEN ONLY ON ONE PLATE; DEFECT?
RV     PIC    MIN II 9.79.
SU     PIC    MIN II 10.4.
DELTA  PIC    MIN II 4.83.
R      PSC    P VAR. MAX=2418070+344.14D*E (J.D.2397070-
              2420000); MAX=2427661+342.1D*E (J.D.2420000-
              27700); MAX=2432866+347.1D*E (J.D.2427300-
              33000); OCE/SINCE J.D.2433000-CM.TA./SEE
              TABLE.
S      PSC    P VAR. MAX=2406665+405.6D*E (J.D.2398944-
              2407100); MAX=2415930+402.6D*E (J.D.2407100-
              16500); MAX=2421295+413.7D*E (J.D.2416500-
              21500); OCE/SINCE J.D.2421500-CM.TA./SEE
              TABLE.
U      PSC    P VAR. MAX=2417230+172.71D*E (J.D.2407720-
              18000); MAX=2423840+174.3D*E (J.D.2418000-24000)
               0001!; MAX=2424527+170.3D*E (J.D.2423000-26100)
               0960!; MAX=2432514+174.05D*E (J.D.2425000-33000)
               0001!; OCE/SINCE J.D.2433000-CM.TA./SEE
              TABLE.
V      PSC    MU ALFA=+0.0112S, MU DELTA=-0.215".
W      PSC    P VAR. MAX=2412690+189.08D*E (J.D.2412692-27100)
               1193!; OCE/SINCE J.D.2435000-CM.TA./SEE
              TABLE.
X      PSC    P VAR. MAX=2429190+352.0D*E (J.D.2416160-29500);
              MAX=2433474+357.3D*E (J.D.2429500-38000); OCE/
              SINCE J.D.2438000-CM.TA./SEE TABLE.
Y      PSC    P VAR. MIN=2410002.844+3.76582D*E (J.D.2410000-
              19700)  9707!; MIN=2425495.522+3.765903D*E
              (J.D.2423200-6300)  1072!; MIN=2430613.384+
              +3.7658895D*E (J.D.2427300-30620); MIN=
              =2432865.357+3.7658405D*E (J.D.2430620-32900);
              MIN=2435693.452+3.7657765D*E (J.D.2432860-
              36600)  0001!; MIN=2441225.473+3.765859D*E (J.D.
              2439000-42500)  6956!; MIN=2443142.29056+
              +3.7658491D*E (J.D.2442500-44000)  8593!; OCE/
              SINCE J.D.2444000-CM.TA./SEE TABLE.
RS     PSC    B PAOHE AAKTK NGC 251./IN THE REGION OF THE
              GALAXY NGC 251.
RT     PSC    CPEH ECK MEHETC C P2=533D./MEAN BRIGHTNESS
              VARIES WITH P2=533D. COACHO/ACCORDING TO  8643!
              30D<P1<70D.
RU     PSC     FE/H!=-1.65. P VAR.  0752, 9714! MAX=2415407.609+
              +0.3903008D*E (J.D.2414400-15700); MAX=
              =2416022.660+0.3902139D*E (J.D.2415700-16600);
              MAX=2417244.537+0.3902878D*E (J.D.2416600-
              19200); MAX=2419936.853+0.3903520D*E
              (J.D.2419200-22000); MAX=2425894.778+0.3903016D*E
              (J.D.2422000-26200); MAX=2426214.829+0.3903546D*E
              (J.D.2426200-27300); MAX=2427397.519:+0.3902216D*E
              (J.D.2427300-28000); MAX=2428165.524+0.3903535D*E
              (J.D.2428000-29300); MAX=2429488.868:+0.3904577D*E
              (J.D.2429300-600)  0752!. MAX=2430053.353+
              +0.390202D*E (J.D.2430000-650); MAX=2430935.366+
              +0.390354D*E (J.D.2430600-940); MAX=2431331.307+
              +0.390457D*E (J.D.2430940-31350); MAX=
              =2432119.417+0.390346D*E (J.D.2431350-32120);
              MAX=2433162.250+0.390283D*E (J.D.2432100-
              33200); MAX=2433905.311+0.390261D*E
              (J.D.2433200-33910); MAX=2433905.311+0.390321D*E
              (J.D.2433900-35430); MAX=2435429.502+0.390412D*E
              (J.D.2435420-35800); MAX=2435781.265+0.39027D*E
              (J.D.2435780-36130); MAX=2436501.361+0.39032D*E
              (J.D.2436130-36510); MAX=2436534.190+0.39043D*E
              (J.D.2436500-36850); MAX=2436845.351+0.39025D*E
              (J.D.2436840-37200); MAX=2437181.358+0.39031D*E
              (J.D.2437180-37610); MAX=2437994.329+0.39026D*E
              (J.D.2437610-38000)  0001!. MAX=2438303.950+
              +0.39040D*E (J.D.2438000-38400)  3879!. MAX=
              =2438375.409+0.39027D*E (J.D.2438370-38650)
               0001!. MAX=2439435.2421+0.390385D*E
              (J.D.2438650-39500)  9713!. MAX=2439435.242+
              +0.390313D*E (J.D.2439430-39800); MAX=
              =2439771.3049+0.39046D*E (J.D.2439770-40140)
               0001!. OCE/SINCE J.D.2440140-CM.TA./SEE
              TABLE. COACHO  3569!, A VAR C P=28.8D./ACCORDING
              TO  3569! A VAR WITH P=28.8D.
RV     PSC    MIN II 12.0.
RY     PSC    (K-B)2=0.03, DS=7. P VAR. MAX=2419677.268+
              +0.52971027D*E (J.D.2414000-22000); MAX=
              =2425148.192+0.52972643D*E (J.D.2422000-25500)
               1337!; MAX=2425508.390+0.5297291D*E
              (J.D.2425500-40000)  3506!; MAX=2441538.476+
              +0.5297291D*E (J.D.2441000-41650)  7984!; OCE/
              SINCE J.D.2442660-CM.TA./SEE TABLE.
RZ     PSC    AOEOOHA./ALGOL-LIKE.
SS     PSC    (K-B)2=0.19; DS=2. EKT AKO/BLAZHKO
              EFFECT:-0.04D<O-C<+0.04D; MIN (O-C)=2437520+
              +136D*E  9731!.
SU     PSC    MIN II 11.3.
SW     PSC    P VAR. MAX=2425177.298+0.5212844D*E (J.D.
              2419670-25200)  4191!; MAX=2425177.256+
              +0.5212642D*E (J.D.2425170-38000)  3506!. OCE/
              SINCE J.D.2438600-CM.TA./SEE TABLE. EMEHT,
              PBEEHHE B TAE, COEPAT CHCOAH
              EH:/THERE IS A PERIODIC TERM IN THE ELEMENTS GIVEN
              IN THE TABLE:+0.0132D SIN 5.440G (E+2). EKT
              AKO/BLAZHKO EFFECT (=34.5D).
SX     PSC    P VAR. MIN=2427811.357+0.825882D*E (J.D.
              2425580-36000)  1218!; MIN=2437202.453+
              +0.825877D*E (J.D.2436000-39900)  0001!; OCE/
              SINCE J.D.2439800-CM.TA./SEE TABLE.
SZ     PSC    MIN II 7.38. P VAR. EMEHT, PBEEHHE B TA-
              E, COEPAT KBAPATH EH:/THERE IS A SQUARE
              TERM IN THE ELEMENTS GIVEN IN THE TABLE:-0.113D*10**-6*E**2.
TY     PSC    PORB=0.080D  9735!. K CBEPXMAKCMMOB -370D/
              THE CYCLE OF SUPERMAXIMA IS 370D  9675!.
UU     PSC    VB A (B 7.60M, F4V, 11.5", 148G, 1966.9). MIN II 6.04;
              MIN II-MIN I=0.55P. BOMOH THOCT OP-
              T  BPAEHE H AC./ELLIPTICAL ORBIT AND
              ROTATION OF THE LINE OF APSIDES ARE POSSIBLE.
UV     PSC    MIN II 9.54. P VAR. MIN I=2424134.574+0.8610475D*E
              (J.D.2414600-24150)  0001!; MIN I=2428038.555+
              +0.861046D*E (J.D.2424150-36700)  2924!; OCE/
              SINCE J.D.2436700-CM.TA./SEE TABLE. OPMA
              KPBO ECKA MEHETC./THE SHAPE OF THE LIGHT
              CURVE VARIES.
UW     PSC    MIN II 11.0:.
UZ     PSC    SB 1 (PORB>1 YR  5751!).
VZ     PSC    MU=0.43", P=65G. MIN II 10.43.
WW     PSC    VB A (B 13.1M, 31").
WX     PSC    OH, H2O, SIO MAEP/MASER.
ZZ     PSC    P1=612S, P2=816S  7476!. HEPAAHE CA-
              /NONRADIAL MODES  8467!.
AG     PSC    P (VR)=0.055D.
AH     PSC    BEA A BHA B 1854-60 .; C 1862 . HE HA-
              AAC./THE STAR WAS SEEN IN 1854-60; SINCE
              1862 IT WAS NOT OBSERVED.
AO     PSC    AHA OXA MAX ECKA. HA KOEAH ECKA C
              PORB=0.1496263D HAKABATC KOEAH C P=
              =858.6861S  BBOE MEHE AMTO (MAX=
              =2444815.00276+0.009938496D*E; M-M=0.54P),
              A TAKE EE OEE CAE KOEAH C P=805.2059S
              (MAX=2444815.00294+0.009319513D*E), KOTOP
              COBAAET C EPOOM PEHTEHOBCKX MCOB,
              OTOECTBEMM C EPOOM BPAEH KOMAKTHO-
              O O'EKTA (O-BMOM, EOO KAPKA)./EPOCH
              OF MAX BRIGHTNESS IS GIVEN. LIGHT VARIATIONS WITH
              PORB=0.1496263D ARE SUPERIMPOSED BY VARIATIONS WITH
              P=858.6861S AND TWICE SMALLER AMPLITUDE (MAX=
              =2444815.00276+0.009938496D*E; M-M=0.54P), AND
              ALSO BY STILL SMALLER OSCILLATIONS WITH P=805.2059S
              (MAX=2444815.00294+0.009319513D*E). THE LAST PE-
              RIOD IS THE X-RAY IMPULSE PERIOD WHICH IS EQUAL TO
              THE PERIOD OF ROTATION OF THE COMPACT OBJECT (PROBABLY
              A WHITE DWARF).
R      PSA    P VAR. MAX=2417385+293.00D*E (J.D.2405000-26000);
              MAX=2432896+291.50D*E (J.D.2426000-38000);
              OCE/SINCE J.D.2438000-CM.TA./SEE TABLE.
S      PSA    P VAR. MAX=2417853+271.0D*E (J.D.2411000-18000);
              MAX=2426880+273.6D (J.D.2418000-27000); MAX=
              =2434714+270.3D (J.D.2427000-35000); OCE/SINCE
              J.D.2434000-CM.TA./SEE TABLE.
X      PSA    MIN II 14.2.
RW     PSA    MIN II 11.63.
TX     PSA    VB B (A 13.0M PG; B 37", 131G); MU=0.22", P=117G.
PI     PSA    SB (PORB=178.3177D  5769!).
R      PUP    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 2439.
U      PUP    P VAR. MAX=2415090+314.26D*E (J.D.2408000-22800);
              OCE/SINCE J.D.2422800-CM.TA./SEE TABLE.
V      PUP    VB A (B 10.0M, 7", 0, 70G; C 11.0M, 19.0", 48G).
              MIN II 4.82. P VAR. IO-CI<0.02D.
W      PUP    P VAR. MAX=2420990+120.68D*E (J.D.2412500-
              23600); MAX=2424725+119.9D*E (J.D.2423600-
              26300); MAX=2432200+120.68D*E (J.D.2426300-
              40800); OCE/SINCE J.D.2440800-CM.TA./SEE
              TABLE.
X      PUP    P VAR. MAX=2414889.8+25.939D*E (J.D.2408800-
              16000); MAX=2435188.76+25.9610D*E (J.D.
              2419000-35190)  2392!; MAX=2436279.50+25.97D*E
              (2435190-38000)  0001!; OCE/SINCE J.D.2438000-
              CM.TA./SEE TABLE.
Z      PUP    OH, H2O, SIO MCC/EMISSION.
              P VAR. MAX=2424256+513.90D*E (J.D.2413900-24500);
              OCE/SINCE J.D.2424500-CM.TA./SEE TABLE.
RS     PUP    OKPEHA OTPAATEHO TMAHHOCT PACOM
              1.4'/SURROUNDED BY THE REFLECTING NEBULOSITY WITH A
              RADIUS OF 1.4'  9634!.
              P VAR. MAX=2419186.3+41.337D*E (J.D.2414000-
              24000)  2049!; MAX=2427083.613+41.414D*E
              (J.D.2425800-28300)  2440!; MAX=2434823.23+
              +41.38535D*E (J.D.2433750-34900)  9636!; OCE/
              SINCE J.D.2435700-CM.TA./SEE TABLE.
RW     PUP    P VAR. MAX=2430175+332.5D*E (J.D.2424500-30200)
               0001!; OCE/SINCE J.D.2435800-CM.TA./SEE
              TABLE.
RX     PUP    PAK KPBO MEHEH ECKA/LIGHT CURVE
              (1890-1925)  1265!.
              MEHEH ECKA KOMOHEHTA TA MP KTA HA-
              ATC B HPAKPACHO OACT CEKTPA:/MIRA
              TYPE COMPONENT LIGHT VARIATIONS ARE OBSERVED IN THE
              INFRARED REGION OF SPECTRUM: MAX=2444530+580D*E,
              3.99M-6.00M J, M-M=0.50P  9518!.
ST     PUP     A/H!=-0.9. OPMA KPBO ECKA  EPO CHO
              MEHTC:/THE LIGHT CURVE SHAPE AND THE PERIOD VA-
              RY STRONGLY: 0.10P<M-M<0.30P; 17.4D<P<19.19D.
              P=19.188D (J.D.2415000-17000); 18.949D (J.D.
              2417000-18000), 18.8065D (J.D.2418000-19000),
              18.721D (J.D.2419000-20000), 18.714D (J.D.2420000-
              21000), 18.717D (J.D.2421000-22000), 18.6175D (J.D.
              2422000-23000), 18.678D (J.D.2423000-24000),
              18.735D (J.D.2424000-25000), 18.796D (J.D.2425000-
              26000), 18.817D (J.D.2426000-27000)  1266!. MAX=
              =2427779.6+18.846D*E (J.D.2427000-28000)  1266!;
              MAX=2428893.9+18.885D*E (J.D.2428000-29000)
               0016!; MAX=2429697.51+19.188D*E (J.D.2429000-
              30000)  1266!. P=19.142D (J.D.2430000-31000),
              19.145D (J.D.2431000-32000)  1266!.
              MAX=2435395.430+18.559D*E (J.D.2435160-500)
               6006!; MAX=2435617.45+18.8864D*E (J.D.2435500-
              5620)  2309!; MAX=243957.3+17.4D*E (J.D.2438700-
              39600)  6611!; OCE/SINCE J.D.2444000-CM.TA./
              SEE TABLE.
SV     PUP    P VAR. MAX=2419010+166.6D*E (J.D.2413660-18000);
              MAX=2423090+169.8D*E (J.D.2418000-23100);
              MAX=2426782+167.8D*E (J.D.2423100-27500);
              OCE/SINCE J.D.2427500-CM.TA./SEE TABLE.
SW     PUP    MIN II 9.1; D=0.029P.
TT     PUP    MIN II 13.6.
TY     PUP    MIN II 8.87.
UZ     PUP    MIN II 10.0.
VV     PUP    MU=0.100", P=165.0G. AHA OXA MAX ECKA. CPE-
              H BEHA MEHETC HA 2-3M. HAATC H-
              TEPBA AKTBHOO MEHEH ECKA C AMT-
              O O 2M P MAKCMAHO CPEHE BEHE. BO
              BPEM HTEPBAOB MAO AKTBHOCT P MHMA-
              HO CPEHE BEHE AMTA OCTAET 0.3M;
              B TO BPEM B HPAKPACHO OACT HAATC
              COAHE MEHEH ECKA CCTEM B PE-
              EAX 15.1M-15.3M J C EMEHTAM
              MIN=2427889.6509+0.0697468256D*E  9644!. EP-
              O BPAEH EOO KAPKA PABEH OPTAHOM
              EPO. MEPAH. OCAHE CEKTPA  9472, 9645!.
              /THE EPOCH OF LIGHT MAXIMUM IS GIVEN. THE MEAN
              BRIGHTNESS VARIES BY 2-3M. INTERVALS OF ACTIVE LIGHT
              VARIATION WITH AMPLITUDE UP TO 2M DURING MAXIMAL ME-
              AN BRIGHTNESS ARE OBSERVED. DURING LOW ACTIVITY INTER-
              VALS WHEN AMPLITUDE IS ABOUT 0.3M MEAN BRIGHTNESS IS
              MINIMAL; DURING THIS TIME THE ELLIPSOIDAL LIGHT VARIA-
              TIONS OF THE SYSTEM ARE OBSERVED IN THE RANGE 15.1M-
              15.3M J WITH THE ELEMENTS MIN=2427889.6509+
              +0.0697468256D*E  9644!. THE WHITE DWARF ROTATION
              PERIOD IS EQUAL TO THE ORBITAL PERIOD. THERE ARE
              FLICKERINGS. SPECTRUM DESCRIPTION  9472, 9645!.
VW     PUP    P VAR. MAX=2425184.67+4.28405D*E (J.D.2422660-
              25600)  0973!; MAX=2435554.86+4.28519D*E (J.D.
              2425600-35600)  2309!; OCE/SINCE J.D.2435500-
              CM.TA./SEE TABLE.
VX     PUP    P1=2.1389D (A1=0.29M); A0=0.31M; P1/P0=0.71042.
VY     PUP    HA MIN II/THE DEPTH OF MIN II 0.04M.
VZ     PUP     A/H!=-0.3. P VAR. MAX=2434864.90+23.1640D*E
              (J.D.2426700-35300)  2309!; OCE/SINCE
              J.D.2435300-CM.TA./SEE TABLE.
WW     PUP    P VAR. MAX=2424497.73+5.5159D*E (J.D.2423520-
              26000)  0973!; OCE/SINCE J.D.2426000-CM.TA./
              SEE TABLE.
WX     PUP    P VAR. MAX=2435042.184+8.93825D*E (J.D.2422000-
              35100)  2431!; OCE/SINCE J.D.2435000-CM.TA./
              SEE TABLE.
WZ     PUP    P VAR. MAX=2427861.33+5.02657D*E (J.D.2421100-
              29400)  2392!; OCE/SINCE J.D.2429400-CM.TA./
              SEE TABLE.
XX     PUP    P VAR. MAX=2426338.503+0.51719805D*E (J.D.
              2426300-39500)  3572!; OCE/SINCE J.D.2441700-
              CM.TA./SEE TABLE.
              (K-B)2=0.07. CEKTPAH KACC-O CAII./THE
              SPECTRAL TYPE ACCORDING TO CA II IS GIVEN.
XY     PUP    MIN II 9.4; D=0.042P.
XZ     PUP    MIN II 7.90. P VAR. MIN I=2440629.7969+2.192383D*E
              (J.D.2425850-41700)  0099!; OCE/SINCE J.D.
              2441700-CM.TA./SEE TABLE.
YY     PUP    HA MIN II/THE DEPTH OF MIN II 0.05M.
AE     PUP    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER CR 173.
AF     PUP    MIN II 13.5.
AG     PUP    MIN II 10.9.
AH     PUP    CM./SEE YY PUP.
AN     PUP    MIN II 10.7.
AQ     PUP    VB A (B 11.13M, <15"; C 12.83M, <15").  A/H!=-0.1.
              AH PEE MEHEH CMMAPHOO ECKA./THE
              RANGE OF THE VARIATION OF COMBINED LIGHT IS GIVEN.
              P VAR. MAX=2429734.59+29.931D*E (J.D.2427500-
              33000)  3474!; MAX=2433296.2+30.018D*E (J.D.
              2433000-35850)  2474!; MAX=2436625.9+29.8568D*E
              (J.D.2435850-36700)  3601!; MAX=2441760.63+
              +30.032D*E (J.D.2436600-42700)  9671!; OCE/
              SINCE J.D.2443400-CM.TA./SEE TABLE.
AR     PUP    CPEH ECK MEHETC C P=1200D./THE MEAN
              BRIGHTNESS VARIES WITH P=1200D.
AS     PUP    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 2546. P VAR. MAX=2416110+
              +331.4D*E (J.D.2415460-26000); OCE/SINCE
              J.D.2426000-CM.TA./SEE TABLE.
AT     PUP    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 2546.
              P VAR. MAX=2426758.205+6.6648D*E (J.D.2426700-
              35600)  2202!; OCE/SINCE J.D.2435600-CM.TA./
              SEE TABLE.
AU     PUP    MIN II 9.28. P VAR. MIN I=2428111.304+1.126418D*E
              (J.D.2414700-28200)  0007!; OCE/SINCE
              J.D.2439000-CM.TA./SEE TABLE.
AV     PUP    MIN II 11.0.
AW     PUP    VB A (B 11.7M, 3.7", 258G). EPO, BOMOHO, CE-
              ET BOT./PERIOD PROBABLY MUST BE DOUBLED.
AY     PUP    MIN II 12.5.
AZ     PUP    MIN II 10.1.
BB     PUP    (K-B)2=0.24; DS=3.
BH_BK  PUP    CM./SEE AE PUP.
BL     PUP    MIN II 14.2.
BN     PUP    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF THE
              OPEN CLUSTER NGC 2533.
BP     PUP    MIN II 12.3.
BQ     PUP    OPMA KPBO ECKA, BOMOHO, MEHETC./THE
              SHAPE OF THE LIGHT CURVE POSSIBLY VARIES.
BR     PUP    MIN II 12.9.
BT     PUP    MIN II 14.5. B PAOHE PACCEHHOO CKOEH/IN THE
              REGION OF THE OPEN CLUSTER NGC 2482.
BU     PUP    MIN II 13.9. B PAOHE PACCEHHOO CKOEH/IN THE
              REGION OF THE OPEN CLUSTER NGC 2447.
BW     PUP    HA MIN II/THE DEPTH OF MIN II 0.15M.
BX     PUP    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 2482.
CE     PUP    P VAR?  7934!.
CH     PUP    P VAR. MAX=2428465+491.0D*E (J.D.2428400-37300);
              OCE/SINCE J.D.2437300-CM.TA./SEE TABLE.
CO     PUP    P VAR? AHA OXA MIN ECKA./THE EPOCH OF LIGHT
              MINIMUM IS GIVEN.
CP     PUP    B 1981 . PAC OOOK, PACPEC CO CKO-
              POCT 710 KM/C, PABEH 7"/IN 1981 THE RADIUS OF THE
              SHELL EXPANDING WITH VEXP=710 KM/S WAS EQUAL TO
              7"  9689, 9559!.
CX     PUP    D=0.05P.
CY     PUP    D=0.01P:; MIN II 13.0.
CZ     PUP    MIN II 13.1.
DD     PUP    MIN II 14.6; MIN II-MIN I=0.572P.
DE     PUP    MIN II 12.9.
DF     PUP    MIN II 12.8.
DK     PUP    MIN II 13.0.
DM     PUP    MIN II 13.7; MIN II-MIN I=0.62P.
DN     PUP    MIN II 13.5.
DO     PUP    MIN II 13.3.
DR     PUP    MIN II 13.3:.
DS     PUP    MIN II 13.4.
DT     PUP    MIN II 14.3.
EK     PUP    VB A (B 15", 270G). P VAR? MAX=2427747.89+
              +2.62587D*E (J.D.2425500-29500)  1343!; OCE/
              SINCE J.D.2434500-CM.TA./SEE TABLE.
EL     PUP    P>1.3D? CM./SEE GI PUP.
EN     PUP    MIN II 11.4.
EQ     PUP    MIN II 10.9.
ES     PUP    COACHO/ACCORDING TO  0412!, MAX=2430377+187D*E.
              EMEHT, PBEEHHE B TAE, OBETBOPT
              HAEHM B HTEPBAE J.D.2425600-29700./THE
              ELEMENTS GIVEN IN THE TABLE ARE VALID IN THE INTERVAL
              J.D.2425600-29700.
EU     PUP    MIN II 14.8.
FK     PUP    A VAR (P2=3000D). B CEKTPE-CHE OOC
              SIC2./STRONG SIC2 BANDS IN THE SPECTRUM.
FM     PUP    MIN II 14.2.
GG     PUP    S5/5.
GH     PUP    VB A (B 10", 195G; C 16", 280G; D 14", 315G). P VAR.
              MAX=2425450+800D*E (J.D.2425300-28000); OCE/
              SINCE J.D.2428700-CM.TA./SEE TABLE.
              OEH KPACHA./VERY RED.
GI     PUP    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 2437.
GK     PUP    CM./SEE GI PUP.
GN     PUP    VB A (B 16.5M, 10", 80G).
GP     PUP    MIN II 13.5.
GU     PUP    MIN II 12.2.
GX     PUP    MIN II 13.9. CM./SEE AE PUP.
GY     PUP    MIN II 12.3.
GZ     PUP    MIN II 12.1.
HH     PUP    (K-B)2=0.14, DS=1.
HI     PUP    MIN II 11.0. CM./SEE AE PUP.
HK     PUP    P VAR. MAX=2425925.732+0.7342532D*E
              (J.D.2425300-36600)  4127!; OCE/SINCE J.D.
              2436600-CM.TA./SEE TABLE.
HM     PUP    ECT HEOK MIN II./THERE IS A SHALLOW MIN II.
HP     PUP    P VAR?
HW     PUP    P VAR? MAX=2429756.28+13.4532D*E (J.D.2427100-
              33000)  3551!; OCE/SINCE J.D.2433000-CM.TA./
              SEE TABLE.
KQ     PUP    B PACCEHHOM CKOEH/IN THE OPEN CLUSTER NGC
              2422. SB 2 (PORB=9752D  3985!).
KT     PUP    MIN II 13.4.
KW     PUP    MIN II 11.8.
KX     PUP    MIN II 13.04; 0.435P (1930)<MIN II-MIN I<0.56P (1973)
               3474, 8094!; E=0.15. BEHE H AC./APSI-
              DAL MOTION.
KY     PUP    MIN II 11.1.
LN     PUP    MIN II 12.9; MIN II-MIN I=0.533P.
LO     PUP    MIN II 13.9.
LP     PUP    D=0.03P:.
LT     PUP    MIN II 12.6.
MN     PUP    MIN II 13.2.
MQ     PUP    MIN II 9.39.
MT     PUP    RCB?
MW     PUP    MIN II 9.2.
NO     PUP    VB A  BC 7.19M V, 8.1". 124G (DM=0.0M, 0.20", 275G,
              1976)!. MIN II 6.66; MIN II-MIN I=0.582P; E=0.123.
NQ     PUP    S 4.5/2-.
NW     PUP    PORB=1D.
NX     PUP    CBAHA C KOMETOOPAHO TMAHHOCT./CONNEC-
              TED WITH A COMETARY NEBULA.
OR     PUP    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 2467.
OS     PUP    VB A (B 6.10M, 67.4"). B PAOHE PACCEHHOO CKOE-
              H/IN THE REGION OF THE OPEN CLUSTER C 0812-362.
OU     PUP    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER IC 2391.
OX     PUP    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF THE
              OPEN CLUSTER NGC 2451.
PS     PUP    HA MIN II/THE DEPTH OF MIN II 0.028M.
PT     PUP    P2=0.168377D. A (LAMBDA 1550)=0.043M; 0.015M<A(B)<
              <0.035M.
PU     PUP    VB (5.2M, 5.6M; 0.11", 43.6G, 1927). MIN II 4.74.
PV     PUP    VB B (A 6.1M; B 16.9", 340G; C 10.5M, 100.4", 228G).
              MIN II 7.31; DII 0.10P; MIN II-MIN I=0.47P.
              OPMA KPBO ECKA B MAX  MIN II MEHETC.
              KOHEH OT CPEHE KPBO DB MEHTC B PEE-
              AX OT -0.06M O +0.03M C EMEHTAM:
              MAX(IDBI)=2440000.027458+1.92207D*E 
              MAX(IDBI)=2440000.219470+0.48003D*E./THE LIGHT
              CURVE SHAPE IN MAX AND MIN II VARIES. THE DEVIATIONS
              DB FROM THE MEAN CURVE VARY FROM -0.06M TO +0.03M
              WITH THE ELEMENTS: MAX (IDBI)=2440000.027458+
              +1.92207D*E OR MAX (IDBI)=2440000.219470+
              +0.48003D*E.
PW     PUP    MIN II 9.54; D=0.095P. CM./SEE R PUP.
QS     PUP    0.008M<A(U)<0.015M.
QT     PUP    BOMOHO, EH PACCEHHOO CKOEH/PROBABLY A
              MEMBER OF THE OPEN CLUSTER NGC 2477.
QU     PUP    P2=0.1680D /OR 0.2019D; 0.010M<A(U)<0.040M.
QV     PUP    BOMOHO, EH PACCEHHOO CKOEH/MAY BE A
              MEMBER OF THE OPEN CLUSTER NGC 2489.
RO     PUP    VB A (B 13.7M, 29.6", 15G).  FE/H!=+0.13. P VAR.
              MAX=2435552.807+0.14088141D*E (J.D.2413900-
              37500)  9756!; MAX=2439887.843+0.14088141D*E
              (J.D.2439800-43700); OCE/SINCE J.D.2444000-CM.
              TA./SEE TABLE.
L2     PUP    VB A (B 11.5M, 62", 214G); MU=0.34", P=18G. H2O, SIO
              MAEP/MASER.
S      PYX    P VAR. MAX=2411770+206.60D*E (J.D.2405500-23700);
              MAX=2423765+207.0D*E (J.D.2423700-29600);
              OCE/SINCE J.D.2429600-CM.TA./SEE TABLE.
T      PYX    PEECTBE BCK HAAC B 1890,
              1902, 1920, 1944  ./PREVIOUS OUTBURSTS WERE OBSER-
              VED IN 1890, 1902, 1920, 1944.
RR     PYX    K CTHK 14.5M./A CLOSE COMPANION 14.5M.
RZ     PYX    MIN II 9.69.
SU     PYX    D=0.016P.
TT     PYX    P=3.031556D?
TV     PYX    HA MIN II/DEPTH OF MIN II 0.05M.
TX     PYX    MIN II 9.8.
TY     PYX    MIN II 7.48.
TZ     PYX    MIN II 11.1.
UZ     PYX    VB A (B 7.61M, 110", 180G).
VV     PYX    VB A (B 8.58M, 0.3"). AH PEE MEHEH CM-
              MAPHOO ECKA./RANGE OF THE VARIATION OF COMBINED
              LIGHT IS GIVEN. MIN II 7.03; DII=0.08P; MIN II-MIN I=
              =0.48P. MIN II=2444622.86709+4.5961766D*E. BPA-
              EHE H AC/APSIDAL MOTION (P=3200 YR.).
VW     PYX    PO AHETAPHO TMAHHOCT K 1-2./THE NUCLEUS
              OF THE PLANETARY NEBULA K 1-2.
              PEE MEHEH CMMAPHOO ECKA:/THE RANGE
              OF THE VARIATIONS OF COMBINED LIGHT: 15.7-17.4 PG.
              AHA OXA MAX ECKA  HAEHE P, KOE K HA-
              EHHOM OHOM  9767!./THE VALUE OF P CLOSE TO
              THAT FOUND BY BOND  9767! AND THE EPOCH OF MAX BRIGHT-
              NESS ARE GIVEN IN THE TABLE.
R      RET    P VAR. MAX=2403013+280.0D*E (J.D.2403000-13900);
              MAX=2423317+276.68D*E (J.D.2413900-25300);
              MAX=2430008+279.7D*E (J.D.2425200-30020);
              OCE/SINCE J.D.2430000-CM.TA./SEE TABLE.
T      RET    CPEH ECK MEHETC C P=200D./MEAN BRIGHTNESS
              VARIES WITH P=200D.
X      RET    (K-B)2=0.09. P VAR. MAX=2427425.47+0.4920D*E
               0357!; MAX=2434334.611+0.492011D*E (J.D.2434300-
              600)  0080!; OCE/SINCE J.D.2434600-CM.TA./
              SEE TABLE.
              OPMA KPBO ECKA MEHETC. EKT AKO:/
              THE SHAPE OF THE LIGHT CURVE VARIES. BLAZHKO EFFECT:
              >45D; 0.13P<M-M<0.23P  0080!.
R      SGE    P VAR (70.07D<P<71.24D  9769!. CCEOBAHE ME-
              HEH EPOA/PERIOD VARIATION STUDY  0767!. EMEH-
              T, PBEEHHE B TAE, OBETBOPT HAE-
              HM OCE J.D.2434000./THE ELEMENTS GIVEN IN THE
              TABLE ARE VALID SINCE J.D.2434000.
              CPEH ECK MEHETC:/THE MEAN BRIGHTNESS VARI-
              ES: MIN=2414402+1112.D*E  1357!.
S      SGE    SB1 (PORB=675D  1358!). P VAR. MAX=2409863.32+
              +8.381968D*E (J.D.2406600-18000); OCE/SINCE
              J.D.2418000-CM.TA./SEE TABLE.
U      SGE    VB A (B 9.6M, 92.0", 318G). MIN II 6.71; 0.014P<DI<
              <0.024P. B PAOHE PACCEHHOO CKOEH COL 399.
              HE EH CKOEH./IN THE REGION OF THE OPEN CLUSTER
              COL 399. NOT A MEMBER OF THE CLUSTER. P VAR  6224,
              8608!. B TAE PBEEH CPEHE EMEHT,
              PECTABE OX MIN C TOHOCT O +-0.008P./
              MEAN ELEMENTS ARE GIVEN IN THE TABLE REPRESENTING
              EPOCHS OF MIN WITHIN +-0.008P. OPMA KPBO ECKA
              MEHETC./THE SHAPE OF THE LIGHT CURVE VARIES.
V      SGE    VB A (B 13.9M, 9.7", 267G); SB 2 (K1=320 KM/C,
              K2=85 KM/C). P VAR? HA ATMEH MEHETC
              OT 0.6M O 1.3M. CPEH ECK BHE ATMEH MEH-
              ETC. HAATC BCK C AMTO O 3M 
              HEOE KTA ECKA C XAPAKTEPHM BPE-
              MEHEM OPKA MHT, ECTKOB MHT  CTOK. O-
              CAHE CEKTPA  3593, 9472!./THE DEPTH OF ECLIPSES
              VARIES FROM 0.6M TO 1.3M. THE MEAN BRIGHTNESS OUTSIDE
              ECLIPSES VARIES. THERE ARE ALSO FLARES WITH AMPLITU-
              DES UP TO 3M AND SMALL LIGHT VARIATIONS WITH A TIME
              SCALE OF MINUTES, DOZENS OF MINUTES AND A FEW DAYS.
              SPECTRUM DESCRIPTION  3593, 9472!.
X      SGE    VB A (B 13.18M, 6", 248G).
Z      SGE    V1 (NGC 6838, M71). EH APOBOO CKOEH/
              GLOBULAR CLUSTER MEMBER. P VAR. MAX=2437870+175.3D*E
              (J.D.2437000-38700); OCE/SINCE J.D.2438700-CM.
              TA./SEE TABLE.
RS     SGE    CPEH ECK MEHETC:/THE MEAN BRIGHTNESS
              VARIES: MAX=2435999+1124D*E  8104!.
              HAAC TAKE BA AOEOOHX OCAEH
              ECKA:/TWO ALGOL-LIKE LIGHT WEAKENINGS WERE ALSO
              OBSERVED: J.D.2444837.22, 2444865.17  9727!.
RW     SGE    P VAR. COACHO/ACCORDING TO  1363! MAX=2424289+
              +429D*E. OCE/SINCE J.D.2434000-CM.TA./SEE
              TABLE.
RZ     SGE    PORB=97M  9771!. CPEH K-COACHO  9785!.
              CBEPXMAKCMM OBTOPTC C KOM 266D. EP-
              O CBEPXOPOB MEHAETC OT 101.3M O 100.8M./
              MEAN CYCLE IS GIVEN ACCORDING TO  9785!. SUPERMAXIMA
              ARE REPEATED WITH THE CYCLE 266D. THE PERIOD OF SUPER-
              HUMPS DECREASES FROM 101.3M TILL 100.8M.
SY     SGE    MIN II 10.7. P VAR. PBEEHHE B TAE EMEHT
              CPABEB B HTEPBAE/ELEMENTS GIVEN IN THE
              TABLE ARE VALID IN THE INTERVAL J.D.2425800-38300.
TU     SGE    D=0.035P.
TX     SGE    P VAR. MAX=2425002+155.0D*E (J.D.2414900-25100);
              OCE/SINCE J.D.2425000-CM.TA./SEE TABLE.
UU     SGE    VB A (B 16.5MB, 4", 90G). PO AHETAPHO TMAH-
              HOCT/THE NUCLEUS OF THE PLANETARY NEBULA ABELL 63.
              MIN II 14.41; D=0.019P. AH PEE MEHEH
              CMMAPHOO ECKA. CTHHA HA MIN I-OKO-
              O 4.3M./THE RANGE OF THE COMBINED LIGHT VARIATION IS
              GIVEN. THE ACTUAL DEPTH OF MIN I IS ABOUT 4.3M.
              OO EKT OTPAEH./LARGE REFLECTION EFFECT.
UZ     SGE    MIN II 11.6:. P VAR. MIN I=2429961.231+2.215750D*E
              (J.D.2429000-41600); OCE/SINCE J.D.2441600-CM.
              TA./SEE TABLE.
VZ     SGE    VB A (B 12M, 28.2", 206G).
WY     SGE    NOVA SGE 1783(MAX J.D.2372494:). MIN I=2445137.8993+
              +0.1536342D*E; D=0.16P. ECK BHE ATMEH-OHO
              -18.7M, HA ATMEH-1.5-2M. B HACTOEE BPEM
              HOA HAATC BCK HA 1.6M, OOHE BC-
              KAM BE TA UG, A TAKE CTPE KTA
              ECKA  9708!/BRIGHTNESS OUTSIDE ECLIPSES IS USUAL-
              LY-18.7M, THE DEPTH OF THE ECLIPSES IS-1.5-2M. AT
              PRESENT OUTBURSTS BY 1.6M ARE SOMETIMES OBSERVED SI-
              MILAR TO THE UG TYPE VARIABLE OUTBURSTS, AS WELL AS
              RAPID FLICKERING OF LIGHT  9708!.
WZ     SGE    NOVA SGE 1913, 1946, 1978. VB A (B 15.76MB, 7",
              280G). B ECTBTEHOCT HE BETC HOBO. O
              CX OP  APECTPPOBAH TP BCK:/
              REALLY IT IS NOT A NOVA. THREE OUTBURSTS WERE REGISTE-
              RED UP TO DAY: J.D.2420094, 32001, 43844  9710, 9711!.
              BO BPEM BCK HAATC OP HA KPBO
              ECKA C 0.057250D>P>0.05714D (A=0.3MV)  9710,
              9776!./THERE ARE SUPERHUMPS ON THE LIGHT CURVE DU-
              RING THE OUTBURST WITH 0.057250D>P>0.05714D (A=0.3MV)
               9710, 9776!.
              ECK ME BCKAM MEHETC (A=0.14M-0.3M).
              P HEKOTOPX OCAEHX ECKA POCXOT A-
              OEOOHE ATMEH HO 0.2M, OBETBOP-
              E EMEHTAM:/THERE ARE LIGHT VARIATIONS BETWEEN
              THE OUTBURSTS (A=0.14M-0.3M). DURING SOME OF LIGHT
              WEAKENINGS ALGOL-LIKE ECLIPSES ARE OBSERVED (A=
              =0.2M) WITH THE ELEMENTS: MIN I=2437547.72845+
              +0.0566878455D*E  9774!; D=0.04P. D=0.02P.
              HAATC TAKE CTPE KOEAH ECKA
              (A<0.01M). EPO TX KOEAH O BCK
              1978 OA COCTAB 28.98S  27.87S  9774!, A OCE
              BCK-28.95963S  9775!. COACHO  9777!, B
              1976-78 . T KOEAH PECTABC EMEH-
              TAM:/THERE ARE ALSO RAPID LIGHT OSCILLATIONS (A<
              <0.01M). THE PERIODS OF THESE OSCILLATIONS BEFORE THE
              1978 OUTBURST WERE 28.98S AND 27.87S  9774!, BUT AF-
              TER THIS OUTBURST-28.95963S  9775!. ACCORDING TO
               9777!, IN 1976-78 THESE OSCILLATIONS WERE REPRESEN-
              TED BY THE ELEMENTS: MAX=2443311.790250+
              +0.00032254826D*E+9.8D*10**-16*E**2.
XY     SGE    COACHO  3705!, CEKTP-OEE PAHH, EM MO./
              ACCORDING TO  3705! THE SPECTRUM IS EARLIER THAN MO.
AG     SGE    P=117D?
BR     SGE    D=0.030P.
CP     SGE    MIN II 13.3.
CU     SGE    MIN II 11.3.
CW     SGE    MIN II 11.7. P VAR? OPMA KPBO ECKA MEHETC./
              THE SHAPE OF THE LIGHT CURVE VARIES.
CZ     SGE    MIN II 15.2.
DH     SGE    OPMA KPBO ECKA MEHETC./THE SHAPE OF THE
              LIGHT CURVE VARIES (1.1M<A<1.7M).
              P VAR. MAX=2427612.509+0.4695844D*E (J.D.2427600-
              38800)  4027!; OCE/SINCE J.D.2438800-CM.TA./
              SEE TABLE. OCE MEHEH EPOA EKT A-
              KO CE/BLAZHKO EFFECT DISAPPEARED AFTER THE PERIOD
              CHANGE (A=1.1M).
DI     SGE    P VAR. MAX=2427929+203.0D*E (J.D.2427500-30200)
               2641!; OCE/SINCE J.D.2437100-CM.TA./SEE
              TABLE.
DK     SGE    MIN II 13.0.
DL     SGE    MIN II 11.5.
DM     SGE    MIN II 11.6.
DP     SGE    P VAR. MAX=2427985.464+0.4883395D*E (J.D.
              2427985-33000); MAX=2432855.191+0.4883339D*E
              (J.D.2433000-40775); OCE/SINCE J.D.2440775-
              CM.TA./SEE TABLE.
DQ     SGE    MIN II 14.8.
DS     SGE    MIN II 16.0:.
DT     SGE    D=0.05P:.
EH     SGE    VB A (B 15.6M).
EI     SGE    MIN II 14.6.
ER     SGE    P VAR. MAX=2430515.460+0.4184209D*E (J.D.
              2427000-38400); MAX=2438443.388+0.4184356D*E
              (J.D.2438400-41800); OCE/SINCE J.D.2441800-CM.
              TA./SEE TABLE.
FF     SGE    D=0.03P; MIN II 13.0.
FG     SGE    VB A (B 14.2M, 8", 100G). B EHTPE AHETAPHO T-
              MAHHOCT PK 60G-7G1 (AMETP 36", BOPACT-6000
              ET). ECK OCTEEHHO BOPACTA C 13.6 PG B
              1894 ., OCT MAKCMMA B 1967 ., OCE EO
              OCTEEHHO MEHAETC, OCTHB 11.0 B B 1982 .
              B 1967 . B CEKTPE OBC MOHE H OO-
              EH PEKOEMEHX EMEHTOB. CEKTPAH
              KACC CTAHOBTC BCE OEE OHM. HAAC
              PHAK BPACBAH HOBO AHETAPHO TMAH-
              HOCT. B 1962 . BEA BOA B OOC HECTA-
              HOCT HA APAMME MV, B-V  HAAA CPOBAT
              C HEOO AMTO  BEBAMC EPO-
              OM: MIN(V)=2442629+59.83D*E+1.126D*E**2
              (J.D.2442600-44530). A 20 ET EPO BOPOC OT
              50D O 134D, AMTA CA MEHAC OT
              0.2MV O 0.5MV, B HACTOEE BPEM BHOB MEH-
              AC O 0.2MV, A EPO COCTABET 90D  9780!./
              THE CENTRAL STAR OF THE PLANETARY NEBULA PK 60G-7G1
              (DIAMETER 36", THE AGE ABOUT 6000 YEARS). THE BRIGHT-
              NESS OF THE STAR STEADILY INCREASED FROM 13.6 PG IN
              1894 TO THE MAXIMUM IN 1967, AND THEN IS STEADILY
              DECREASING. IN 1982 IT WAS 11.0 B. IN 1967 THE STRONG
              ABSORPTION LINES OF RARE EARTH ELEMENTS APPEARED IN
              THE SPECTRUM. THE SPECTRAL CLASS STEADILY BECOMES
              LATER. THE SIGNES OF NEW PLANETARY NEBULA EJECTION WE-
              RE OBSERVED. IN 1962 THE STAR ENTERED THE INSTABILITY
              STRIP IN THE MV, B-V DIAGRAM AND BEGAN TO PULSATE
              WITH A SMALL AMPLITUDE AND INCREASING PERIOD: MIN(V)=
              =2442629+59.83D*E+1.126D*E**2 (J.D.2442600-44530).
              IN TWENTY YEARS THE PERIOD INCREASED FROM 50D TO 134D,
              THE AMPLITUDE OF PULSATIONS CHANGED FROM 0.2MV TO
              0.5MV; NOW IT DECREASED AGAIN TO 0.2MV, AND THE PE-
              RIOD IS ONLY 90D  9780!.
FH     SGE    MIN II 13.5.
FL     SGE    K CTHK 14M. B MHMME, BOMOHO, CA-
              EE 15.9M./THERE IS A CLOSE COMPANION 14M. IN THE
              MINIMUM PROBABLY FAINTER THAN 15.9M.
FO     SGE    P VAR. MAX=2427578.0+67.8D*E (J.D.2427570-28120);
              MAX=2428134.4+72.7D*E (J.D.2428120-30150); OC-
              E/SINCE J.D.2430150-CM.TA./SEE TABLE.
FP     SGE    MIN II 14.9. P=0.32100275D?
FT     SGE    P.K.55-1G2. HE AHETAPHA TMAHHOCT./NOT A PLA-
              NETARY NEBULA.
FU     SGE    MIN II 15.8.
FX     SGE    B PAOHE APOBOO CKOEH/IN THE REGION OF THE
              GLOBULAR CLUSTER M71 (NGC 6838).
GI     SGE    KPACHA./RED.
GN     SGE    MIN II 10.6.
GP     SGE    KPACHA./RED.
GY     SGE    P VAR. MAX=2431264.49+51.497D*E (J.D.2429490-
              34900)  7199!; MAX=2433787.42+51.5991D*E (J.D.
              2433600-37280), MAX=2437911.04+51.2594D*E
              (J.D.2437280-40510)  6172!; OCE/SINCE
              J.D.2444450-CM.TA./SEE TABLE.
HH     SGE    HAATC K 23-26D  300D./THE CYCLES
              23-26D AND 300D ARE OBSERVED.
HM     SGE    VB A (B 14.20M, 10", 182G). BEEHE ECKA OT
              17.2M O 11.3M PG POOO B HTEPBAE
              J.D.2442280-42650. OCE TOO B HPAKPACHX
              AX HAATC KOEAH ECKA C P=550D
               9721, 9783!  A(K)=1.5M. CTOHK PAO-  PEHT-
              EHOBCKOO EH./THE BRIGHTNESS INCREASED
              FROM 17.2M UP TO 11.3M PG IN THE INTERVAL J.D.2442280-
              42650. THEN THE LIGHT VARIATIONS IN THE INFRARED REGION
              APPEARED WITH P=550D  9721, 9783! AND A(K)=1.5M.
              RADIO AND X-RAY SOURCE.
IR     SGE    SF BEA B TECHO APE./SF STAR IN A CLOSE PAIR.
LN     SGE    CM./SEE IR SGE.
MV     SGE    BOMOH EH APOBOO CKOEH./POSSIBLE MEM-
              BER OF THE GLOBULAR CLUSTER PALOMAR 10.
MZ     SGE    CM./SEE MV SGE.
PT     SGE    P KOMOHEHT TECHO AP./P COMPONENT OF A CLOSE
              PAIR.
DELTA  SGE    VB A (B, A=0.04", P=7 YR); SB 2 (PORB=3725D  9789!).
              OCEHEE BEPXHEE COEHEHE B-BE  EE AT-
              MOCEPHOE ATMEHE POOO B MAPTE-APEE
              1980 ./THE LAST SUPERIOR CONJUNCTION OF THE B-STAR
              AND   ITS ATMOSPHERIC ECLIPSE WAS IN MARCH-APRIL
              1980  9726!.
R      SGR    P VAR. MAX=2405776+271.0D*E (J.D.2399500-
              2407500); MAX=2407115+264.2D*E (J.D.2407100-
              9500); MAX=2418125+269.65D*E (J.D.2409500-
              19500); MAX=2433137+267.90D*E (J.D.2419500-
              36000); OCE/SINCE J.D.2436000-CM.TA./SEE
              TABLE.
S      SGR    P VAR. MAX=2401029+230.6D*E (J.D.2401000-10000);
              MAX=2411638+229.2D*E (J.D.2410000-19500);
              MAX=2422222+232.81D*E (J.D.2419500-27000);
              OCE/SINCE J.D.2427000-CM.TA./SEE TABLE.
T      SGR    CTHK/COMPANION F3IV (RO<0.8"). P VAR. MAX=
              =2409013+385.1D*E (J.D.2401500-10500); MAX=
              =2414582+399.0D*E (J.D.2413000-17500); MAX=
              =2424363+387.9D*E (J.D.2417500-25500); OCE/
              SINCE J.D.2425500-CM.TA./SEE TABLE.
              S 5/6-E. B CEKTPE-H TC  OEH HTEHCBHA
              H LI LAMBDA 6708./THERE ARE TC LINES AND A VERY STRONG
              LI LAMBDA 6708 LINE IN THE SPECTRUM.
U      SGR    EH PACCEHHOO CKOEH/THE MEMBER OF THE OPEN
              CLUSTER M25 (IC 4725).
              P VAR. MAX=2416628.046+6.744925D*E (J.D.2404480-
              30115)  0765!; OCE/SINCE J.D.2430115-CM.TA./
              SEE TABLE.  A/H!=0.1.
W      SGR    VB A (A 9.2M, 0.116", 153.3G, 1976.477; B 13.5M, 33.4",
              233G; C 13.5M, 47.9", 101G). P VAR. MAX=2403198.39+
              +7.594695D*E (J.D.2403100-34500); OCE/SINCE
              J.D.2434500-CM.TA./SEE TABLE.
X      SGR    P VAR. MAX=2410006.22+7.01206D*E (J.D.2403000-
              17000); MAX=2424248.11+7.01245D*E (J.D.2417000-
              34500); OCE/SINCE J.D.2434500-CM.TA./SEE
              TABLE.
Y      SGR    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER M25 (IC 4725).
RR     SGR    P VAR. MAX=2410008+336.0D*E (J.D.2410000-17100)
               9794!; MAX=2422755+332.73D*E (J.D.2422700-
              32100)  0960!; OCE/SINCE J.D.2432100-CM.TA./
              SEE TABLE. OH, H2O MCC/EMISSION.
RS     SGR    VB A (B 9.65MV, 39.0", 86G). MIN II 6.28.
RT     SGR    P VAR. MAX=2412759+303.1D*E (J.D.2412700-8300)
               0960!; MAX=2425588+308.8D*E (J.D.2422800-26700);
              MAX=2428034+303.8D*E (J.D.2426700-33500);
              OCE/SINCE J.D.2433500-CM.TA./SEE TABLE.
RU     SGR    P VAR. MAX=2413062+242.3D*E (J.D.2410150-16700)
               0960!; MAX=2423670+242.3D*E (J.D.2422500-
              24500); MAX=2428200+237.6D*E (J.D.2424500-
              28800); OCE/SINCE J.D.2428800-CM.TA./SEE
              TABLE.
RV     SGR    P VAR. MAX=2411206+319.3D*E (J.D.2410200-17000)
               0960!; MAX=2429032+321.3D*E (J.D.2422600-
              29500); OCE/SINCE J.D.2429500-CM.TA./SEE
              TABLE.
RW     SGR    P VAR. MAX=2413798+189.0D*E (J.D.2413700-23000);
              MAX=2431998+190.87D*E (J.D.2423000-33500);
              OCE/SINCE J.D.2433500-CM.TA./SEE TABLE.
RX     SGR    P VAR. MAX=2417730+330.3D*E (J.D.2413000-18500);
              MAX=2420122+346D*E (J.D.2418500-20150); MAX=
              =2420122+323D*E (J.D.2420100-22200); MAX=
              =2424120+345D*E (J.D.2422200-24200); MAX=
              =2428785+332.2D*E (J.D.2424000-31500); OCE/
              SINCE J.D.2431500-CM.TA./SEE TABLE.
RY     SGR    VB A (B 15.69M, 12"). HAATC CAOHHE
              MEHEH ECKA (0.1M<A<1.5M) C EMEHTAM:/
              THERE ARE PULSATIONAL LIGHT VARIATIONS (0.1M<A<1.5M)
              WITH THE ELEMENTS: MAX=2433670+38.6056D*E-
              -78D*10**-5*E**2.
              KPBE MEHEH ECKA  9798, 9799!; OCAHE
              CEKTPA  6261!./LIGHT CURVE  9798, 9799!; SPECTRUM
              DESCRIPTION  6261!.
ST     SGR    S 6/3-E.
SU     SGR    VB A (B 13.5M, 1.0", 240G, 1932.45). PAHEE HAA-
              C P=88D  0017!./EARLIER P=88D WAS OBSERVED  0017!.
SV     SGR    B TMAHHOCT/IN THE NEBULA M8 (NGC 6523).
SW     SGR    P VAR. MAX=2416338+290.3D*E (J.D.2414000-16500);
              MAX=2428507+288.5D*E (J.D.2422500-29000);
              MAX=2429088+293.5D*E (J.D.2429000-33000);
              OCE/SINCE J.D.2433000-CM.TA./SEE TABLE.
SX     SGR    MIN II 9.62; D=0.05P. P VAR. MIN I=2429114.249+
              +4.15395762D*E (J.D.2410000-29150)  0007!; OCE/
              SINCE J.D.2429000-CM.TA./SEE TABLE.
SY     SGR    B PAOHE TMAHHOCT/IN THE REGION OF THE NEBULA
              S 188.
SZ     SGR    VB A (B 12.5MV, 2.0", 212G).
VV     SGR    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6494.
              OH, H2O MCC/EMISSION.
VX     SGR    P VAR; 1M<A<6M. SIO, H2O, OH MAEP/MASER.
              KPBA ECKA/LIGHT CURVE (1935-1969)  6615!.
VY     SGR     A/H!=0.5.
WX     SGR    VB A (B 12.5M, 0.4", 88G). P VAR. MIN=2419317.259+
              +2.129095D*E (J.D.2419300-24700)  0457!; MIN=
              =2424729.418+2.129113D*E (J.D.2424700-39700)
               0279!; OCE/SINCE J.D.2440000-CM.TA./SEE
              TABLE.
WY     SGR    MIN II 10.3.
WZ     SGR    EH PACCEHHOO CKOEH/THE MEMBER OF THE OPEN
              CLUSTER C 1814-190.  A/H!=0.4.
XX     SGR    P VAR. MAX=2419189.730+6.424264D*E (J.D.2419100-
              30100)  0637!; OCE/SINCE J.D.2435000-CM.TA./
              SEE TABLE.
XZ     SGR    MIN II 8.95; D=0.022P. P VAR. MIN I=2420311.519+
              +3.275537D*E (J.D.2420300-28000)  1604!; MIN I=
              =2436440.137+3.27549D*E (J.D.2428000-37500)
               2516!; MIN I=2441150.348+3.2755357D*E (J.D.
              2437500-41500)  7084!; OCE/SINCE J.D.2441500-
              CM.TA./SEE TABLE.
YY     SGR    MIN II 10.64; MIN II=2433075.8296+2.628463D*E
               2302!. EPO BPAEH H AC-300 ET./
              APSIDAL MOTION PERIOD IS ABOUT 300 YEARS.
AL     SGR    P VAR. MAX=2425792+79.07D*E (J.D.2421000-26000);
              OCE/SINCE J.D.2426000-CM.TA./SEE TABLE.
AN     SGR    P VAR. MAX=2425720+339.62D*E (J.D.2415000-26000);
              MAX=2428360+330.0D*E (J.D.2426000-28500);
              OCE/SINCE J.D.2428500-CM.TA./SEE TABLE.
AP     SGR    SB?  9004!.
AR     SGR    EMEHT COEPAT KBAPATH EH:/THERE IS A
              SQUARE TERM IN THE ELEMENTS:- 0.0031D (E-30)**2+8.8D!.
AS     SGR    AHETAPHA TMAHHOCT/PLANETARY NEBULA HB 6=
              =7+1G1.
AU     SGR    B PAOHE PACCEHHOO CKOEH  HO T-
              MAHHOCT/IN THE REGION OF THE OPEN CLUSTER AND THE
              DIFFUSE NEBULA NGC 6514 (M20).
AV     SGR    B PAOHE PACCEHHOO CKOEH NGC 6546. HE EH
              CKOEH./IN THE REGION OF THE OPEN CLUSTER NGC
              6546. NOT A MEMBER OF THE CLUSTER.
               A/H!=0.4. P VAR. MAX=2429083.30+15.4093D*E
              (J.D.2421400-39100); OCE/SINCE J.D.2439100-
              CM.TA./SEE TABLE.
AW     SGR    VB A (B 16M, 15", 97G). B PAOHE PACCEHHOO CKO-
              EH/IN THE REGION OF THE OPEN CLUSTER NGC 6546.
AY     SGR     A/H!=0.2.
BB     SGR    VB A (B=V4088 SGR, 7.49M-7.87M, 93.5", 102G).
              B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER CR 394.
BE     SGR    A VAR (0.6M<A<1.1M).
BM     SGR    P VAR.
BN     SGR    MIN II 9.37; D=0.04P:. MKOE PEHTEHOBCKOE E-
              HE./SOFT X-RAY SOURCE. P VAR  1600!.
BQ     SGR    D=0.017P. P VAR. MIN=2412592.7905+8.01964D*E
              (J.D.2412590-22220)  1696!; OCE/SINCE J.D.
              2422220-CM.TA./SEE TABLE.
CC     SGR    B PAOHE APOBOO CKOEH/IN THE REGION OF THE
              GLOBULAR CLUSTER NGC 6723.
CD     SGR    CM./SEE CC SGR. P VAR. MAX=2416247+266.62D*E
              (J.D.2411000-23000); OCE/SINCE J.D.2423000-CM.
              TA./SEE TABLE.
CE     SGR    CM./SEE CC SGR.
              SF KOMOHEHT TECHO AP./SF COMPONENT OF A CLOSE
              DOUBLE.
CF     SGR    CM./SEE CC SGR.
              P VAR. MAX=2415632.81+0.570026D*E (J.D.2411000-
              23800)  1616!; OCE/SINCE J.D.2423900-CM.TA./
              SEE TABLE.
CG     SGR    CM./SEE CC SGR.
DH     SGR    B PAOHE APOBOO CKOEH/IN THE REGION OF THE
              GLOBULAR CLUSTER NGC 6809 (M55).
DI-DK  SGR    CM./SEE DH SGR.
DM     SGR    CM./SEE DH SGR.
DO-DP  SGR    CM./SEE DH SGR.
DR-DS  SGR    CM./SEE DH SGR.
DV     SGR    D=0.044P.
EG     SGR    D=0.010P.
FV     SGR    P VAR. MAX=2424010+269.5D*E (J.D.2424000-27500)
               0251!; OCE/SINCE J.D.2427500-CM.TA./SEE
              TABLE.
GG     SGR    P VAR. MAX=2413840+286.5D*E (J.D.2413800-24000);
              OCE/SINCE J.D.2424000-CM.TA./SEE TABLE.
GK     SGR    COACHO  5869!-ATMEHHA./ACCORDING TO  5869!-
              ECLIPSING.
GU     SGR    HAATC TAKE KOEAH ECKA C/THERE ARE
              ALSO LIGHT VARIATIONS WITH<P>=37.5D, 0.4M<A(V)<
              1.5M  6273!.
HH     SGR    VB (RO=0.1').
IR     SGR    VB B (A 13.6M; B 10", 220G).
KO     SGR    OXOA HA UG. BOMOHO, HAEH B MIN ECKA
              OTHOCTC K CTHK./SIMILAR TO UG. IT IS POSSIBLE
              THAT THE OBSERVATIONS IN MIN BRIGHTNESS REFER TO A
              COMPANION.
LZ     SGR    VB A (B 16M, 7", 30G).
MV     SGR    OEH OPA EHA BOOPOOM EPOHO-E-
              BA BEA./VERY HOT HYDROGEN DEFICIENT EXTREME HE-
              LIUM CARBON STAR.
MW     SGR    P VAR. MAX=2418940+202.3D*E (J.D.2418900-23900);
              MAX=2428753+206.5D*E (J.D.2423900-28950); OCE/
              SINCE J.D.2428950-CM.TA./SEE TABLE.
NP     SGR    BOMOH K 100-300D./THE CYCLES 100-300D
              ARE POSSIBLE.
OW     SGR    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6716.
V348   SGR    VB A (B 15M PG, 16", 73G). CM./SEE MV SGR.
              O XAPAKTEP MEHEH ECKA  CEKTP HKA-
              HA. KPBA ECKA HAOMHAET KPBE ECKA BE
              TA RCB; HA HEE HAKABATC HATEHE HE-
              PABHE  OPABHE MEHEH CO CPEHM
              KOM OKOO 200D  2449, 9824!. OKPEHA TMAH-
              HOCT PACOM OKOO 1". OEE CAA TMAHHA
              OOOKA POCEBAETC O 7" OT BE. CH
              HPAKPACH TOK EH. OCAHE CEKT-
              PA  2451, 9825!. O-BMOM, AHMAET POME-
              TOHOE OOEHE ME EPEMEHHM TA RCB
               BEAM TA BOA-PAE, BMC PA-
              M AHETAPHX TMAHHOCTE./BY THE CHARACTER OF
              LIGHT VARIATION AND THE SPECTRUM THE STAR IS UNIQUE.
              THE LIGHT CURVE RESEMBLING THOSE OF RCB TYPE STARS
              IS SUPERIMPOSED BY CONSPICUONS IRREGULAR AND SEMIRE-
              GULAR VARIATIONS WITH THE MEAN CYCLE ABOUT 200D
               2449, 9824!. THE STAR IS SURROUNDED BY A NEBULA THE
              RADIUS OF WHICH EQUALS 1". A FAINTER NEBULOUS ENVELO-
              PE IS OBSERVED UP TO 7" FROM THE STAR. LARGE INFRARED
              EXCESS. SPECTRUM DESCRIPTION  2451, 9825!. PROBABLY
              THE STAR IS INTERMEDIATE BETWEEN THE RCB VARIABLES
              AND PLANETARY NEBULA WOLF-RAYET CENTRAL STARS.
V350   SGR    SB  9004!.
V354   SGR    D=0.02P.
V356   SGR    MIN II 7.24; DII=0.20P:; D=0.05P;
              0.490P (1928)<MIN II-MIN I<0.505P (1951). BOMO-
              HO BEHE H AC./APSIDAL MOTION IS POSSIBLE.
V366   SGR    P VAR. MAX=2425479.448+0.4779616D*E (J.D.
              2423990-28780)  0705!; OCE/SINCE J.D.2435600-
              CM.TA./SEE TABLE.  CA/H!=-0.73.
V367   SGR     CA/H!=-1.21.
V377   SGR    B TAE AHA OXA MIN ECKA./THE EPOCH OF
              LIGHT MIN IS GIVEN IN THE TABLE.
              P VAR. MIN=2426071.24+16.17076D*E (J.D.2425300-
              26600)  0048!; MIN=2427350.25+16.19326D*E (J.D.
              2426600-28700)  1400!; MIN=2436358.98+16.1575D*E
              (J.D.2436200-37300); MIN=2437863.09+16.1925D*E
              (J.D.2437660-39100); MIN=2440114.81+16.2407D*E
              (J.D.2440200-560); OCE/SINCE J.D.2440950-CM.
              TA./SEE TABLE.
V397   SGR    EMEHT COEPAT KBAPATH EH:/THERE IS A
              SQUARE TERM IN THE ELEMENTS:-0.009D*10**-6*E**2
V401   SGR    MIN II 14.1.
V403   SGR    EMEHT COEPAT KBAPATH EH:/THERE IS A
              NONLINEAR TERM IN THE ELEMENTS:-0.013D*10**-6*E**2.
V410   SGR    VB A (B 13.6M, 270G).
V426   SGR    MIN II 13.3.
V427   SGR    EMEHT COEPAT KBAPATH EH:/THERE IS A
              NONLINEAR TERM IN THE ELEMENTS:-131D*10**-10*E**2.
              OPMA KPBO ECKA MEHETC:/THE SHAPE OF THE
              LIGHT CURVE VARIES: 0.17P<M-M<0.22P.
V431   SGR    MIN II 14.9.
V437   SGR    MIN II 14.0.
V440   SGR    DS=9. P VAR. P=0.4774659D (J.D.2416000-23000)
               0752!; P<0.4774659D (J.D.2422000-26000)  0235!;
              MAX=2426581.203+0.477474D*E (J.D.2426000-29460)
               1000!; OCE/SINCE J.D.2437100-CM.TA./SEE
              TABLE.
V453   SGR    EMEHT COEPAT KBAPATH EH:/THERE IS A
              NONLINEAR TERM IN THE ELEMENTS:+0.003D*10**-6*E**2.
V457   SGR    EMEHT COEPAT KBAPATH EH:/THERE IS A
              NONLINEAR TERM IN THE ELEMENTS:-0.005D*10**-6*E**2.
V466   SGR    EMEHT COEPAT KBAPATH EH:/THERE IS A
              NONLINEAR TERM IN THE ELEMENTS:+0.03D*10**-6*E**2.
V496   SGR    MIN II 14.3.
V497   SGR    MIN II 16.0.
V505   SGR    MIN II 6.63. P VAR. MIN I=2433515.3295+1.18287141D*E
              (J.D.2425500-35800)  1642!; MIN I=2437494.4964+
              +1.1828622D*E (J.D.2435800-37500); MIN I=
              =2440055.3991+1.1828650D*E (J.D.2437500-40100);
              MIN I=2442656.5283+1.18286917D*E (J.D.2440100-
              42670); OCE/SINCE J.D.2442670-CM.TA./SEE
              TABLE.
              OPMA KPBO ECKA MEHETC. OTKOHEH OT
              CPEHE KPBO ECKA MEHTC C P=310D. PA-
              HOCT H MIN I  MIN II MEHETC HA 0.05M/THE
              SHAPE OF THE LIGHT CURVE VARIES. DEVIATIONS FROM THE
              MEAN LIGHT CURVE VARY WITH P=310D. THE DIFFERENCE
              OF MIN I AND MIN II DEPTHS VARIES BY 0.05M  9830!.
V511   SGR    P VAR. MAX=2423950+158.8D*E (J.D.2411300-23950);
              OCE/SINCE J.D.2423950-CM.TA./SEE TABLE.
V515   SGR    EMEHT COEPAT KBAPATH EH:/THERE IS A
              NONLINEAR TERM IN THE ELEMENTS:+0.015D*E**2.
V519   SGR    EMEHT COEPAT KBAPATH EH:/THERE IS A
              NONLINEAR TERM IN THE ELEMENTS:+0.0046D*E**2.
V520   SGR    EMEHT COEPAT KBAPATH EH:/THERE IS A
              NONLINEAR TERM IN THE ELEMENTS:+0.051D*E**2.
V523   SGR    MIN II 9.88. HAAETC BPAEHE H AC. B
              TAE PBEEHA OXA MIN I, COOTBETCTBA
              MOMEHT COEHEH H AC C OM PEH,
              KOA MIN II-MIN I=0.50P. EPO AH CPEH
              COACHO  2453!, A  EMEP OOX M-
              HMMOB OTKOHEH O-C, HE PEBAE +-0.06P.
              EPO BPAEH H AC COCTABET 248 ET
               2453!. B 1953 . MIN II-MIN I=0.39P./APSIDAL MO-
              TION IS OBSERVED. IN THE TABLE THE EPOCH OF MIN I IS
              GIVEN CORRESPONDING TO THE MOMENT OF LINE OF APSIDES
              COINCIDING WITH THE LINE OF SIGHT, WHEN MIN II-MIN I=
              =0.50P. THE MEAN PERIOD ACCORDING TO  2453! IS GIVEN;
              WITH THIS PERIOD O-C DEVIATIONS DO NOT EXCEED +-0.06P
              FOR BOTH MINIMA. THE PERIOD OF APSIDAL MOTION IS 248
              YEARS  2453!. MIN II-MIN I=0.39P IN 1953.
V524   SGR    MIN II 11.2.
V525   SGR    MIN II 8.51.
V526   SGR    VB A (B 12.40M, 8.6", 7.3G). MIN II 10.20, DII=0.17P;
              DI=0.006P, DII=0.013P.
              EMEHT COEPAT CHCOAHE EH:/THERE
              ARE PERIODIC TERMS IN THE ELEMENTS:
              +0.1369D SIN (0.01295G*E)-0.0115D SIN (0.0259G*E)+
              +0.0011D SIN(0.0388G*E). MIN II=2422055.0453+
              +1.919411D*E-0.1369D SIN (0.01295G*E)-
              -0.0115D SIN (0.0259G*E)-0.0011D SIN (0.0388G*E).
              EPO BPAEH H AC 146 ET./THE PERIOD
              OF APSIDAL MOTION IS 146 YEARS. E=0.224.
V527   SGR    P VAR. MAX=2426904.95+1.258956D*E (J.D.2425790-
              7650)  1648!; OCE/SINCE J.D.2438200-CM.TA./
              SEE TABLE.
V551   SGR    VB B (A 16.5M; B 12", 135G).
V552   SGR    P VAR. PBEEHHE EMEHT CPABEB OCE
              J.D.2418400./THE ELEMENTS GIVEN IN THE TABLE ARE
              VALID SINCE J.D.2418400.
V554   SGR    MIN II 14.5.
V557   SGR    P VAR. MAX=2415110.5+16.233D*E (J.D.2415100-
              22000); MAX=2426100.0+16.260D*E (J.D.2423900-
              27700)  0251!; MAX=2428097.70+16.171D*E (J.D.
              2427700-28800)  0296!; OCE/SINCE J.D.2428800-
              CM.TA./SEE TABLE.
V558   SGR    MIN II 14.3.
V564   SGR    P VAR. MAX=2424056+27.8D*E (J.D.2423780-26000)
               0251!; MAX=2428403.3+27.99D*E (J.D.2427870-
              29160)  0296!; MAX=2429158.2+27.2D (J.D.2429150-
              515); OCE/SINCE J.D.2429515-CM.TA./SEE
              TABLE.
V567   SGR    EHTPAHA BEA AHETAPHO TMAHHOCT/THE
              CENTRAL STAR OF THE PLANETARY NEBULA P.K.355-6G1
              (M3-21).
V573   SGR    MIN II 12.7.
V574   SGR    MIN II 14.7.
V578   SGR    COACHO/ACCORDING TO  2448!, MAX=2428710+
              +253D*E.
V593   SGR    P VAR. MAX=2414150+230D*E (J.D.2414100-22900);
              OCE/SINCE J.D.2423900-CM.TA./SEE TABLE.
V598   SGR    D=0.05P.
V611   SGR    P VAR. MAX=2414150+123D*E (J.D.2414150-19000);
              OCE/SINCE J.D.2420250-CM.TA./SEE TABLE.
              BOMOHO, EPO HAO BOT, TAK KAK BEA HA-
              OMHAET RV TAU (MIN II 16.2)./THE PERIOD MUST PRO-
              BABLY BE DOUBLED BECAUSE THE STAR RESEMBLES RV TAU
              (MIN II 16.2).
V612   SGR    P VAR. MAX=2413750+107.9D*E (J.D.2413700-17900);
              OCE/SINCE J.D.2418800-CM.TA./SEE TABLE.
V615   SGR    P.K.356-7G1=HE 2-349.
V626   SGR    P VAR? MAX=2427715.4+26.745D*E (J.D.2425380-
              28800)  0046!; OCE/SINCE J.D.2434500-CM.TA./
              SEE TABLE.
V631   SGR    MIN II 14.2.
V632   SGR    P VAR. MAX=2413350+263D*E (J.D.2413300-19000);
              OCE/SINCE J.D.2420200-CM.TA./SEE TABLE.
V633   SGR    P VAR. MAX=2415110+224D:.E (J.D.2415000-18800);
              OCE/SINCE J.D.2420000-CM.TA./SEE TABLE.
V638   SGR    P VAR? MAX=2412670+73.1D*E (J.D.2412600-14540);
              OCE/SINCE J.D.2414800-CM.TA./SEE TABLE.
V646   SGR    P VAR. MAX=2413350+95D*E (J.D.2413300-15900);
              OCE/SINCE J.D.2423900-CM.TA./SEE TABLE.
V660   SGR    P VAR. MAX=2426460+235.6D*E (J.D.2426400-35700)
               0251!; OCE/SINCE J.D.2435600-CM.TA./SEE
              TABLE.
V663   SGR    P VAR. MAX=2426160+305D*E  0251!; OCE/SINCE
              J.D.2435600-CM.TA./SEE TABLE.
V671   SGR    P=292.5D?
V672   SGR    P VAR? MAX=2424680+228D*E  0251!; OCE/SINCE
              J.D.2435600-CM.TA./SEE TABLE.
V674   SGR    P VAR. MAX=2425830+249D*E  0251!; OCE/SINCE
              J.D.2435600-CM.TA./SEE TABLE.
V675   SGR    (K-B)2=-0.01; DS=11.
V676   SGR    P VAR. MAX=2414140+181D*E (J.D.2414100-22600)
               0251!; OCE/SINCE J.D.2423900-CM.TA./SEE
              TABLE.
V679   SGR    P VAR. MAX=2415900+225D*E (J.D.2415900-22200)
               0251!; MAX=2425440+223.1D*E (J.D.2425000-
              29000); OCE/SINCE J.D.2429000-CM.TA./SEE
              TABLE.
V683   SGR    MIN II 12.5.
V686   SGR    P VAR? MAX=2425390+225.3D*E  0251!; OCE/SINCE
              J.D.2435600-CM.TA./SEE TABLE.
V687   SGR    MIN II 12.2.
V691   SGR    P VAR? MAX=2426095.550+0.46911D*E  0251!; OCE/
              SINCE J.D.2435630-CM.TA./SEE TABLE.
V703   SGR    VAR 4. COACHO  2951! PEE MEHEH ECKA,
              T EPEMEHHOCT  EMEHT MEHEH ECKA B
               1640! OOHO PCAH BEE VAR 3./ACCORDING
              TO  2951! THE RANGE OF LIGHT VARIATION, THE TYPE OF VA-
              RIABILITY AND THE ELEMENTS OF LIGHT VARIATION ARE ERRO-
              NEOUSLY ASSIGNED IN  1640! TO THE STAR VAR.3.
V705   SGR    MIN II 12.9.
V710   SGR    P VAR. MIN=2426101.550+2.3817D*E  0251!; MIN=
              =2431286.425+2.381633D*E (J.D.2428390-35700)
               3513!.
V713   SGR    P VAR? MAX=2424680+253.4D*E  0251!; OCE/SINCE
              J.D.2435600-CM.TA./SEE TABLE.
V716   SGR    P VAR? MAX=2424670+277D*E  0251!; OCE/SINCE
              J.D.2435600-CM.TA./SEE TABLE.
V718   SGR    P VAR? MAX=2425850+153.2D*E  0251!; OCE/SINCE
              J.D.2435600-CM.TA./SEE TABLE.
V721   SGR    P=71:D?
V725   SGR    HKAHA BEA. CPEH BEHA BOPOCA C
              13.0M O 12.4M C 1889 O 1915 .  AA O 12.8M B
              1926 . C 1895 . O 1926 . PEAHE KOPOTKOEPO-
              ECKE KOEAH C AMTO OKOO 0.4M. B
              1928 . AMTA BHEAHO BOPOCA OT HA 2M,
              P TOM BEHA B MAKCMME HE MEHAC. C
              1928 . O 1935 . MEHEH ECKA CTA EPO-
              ECKM, PEM EPO C KAM OOM BE-
              BAC HA 1D B COOTBETCTB C OPMO: MIN=
              =2426087+15.933D*E+0.0233D*E**2. B 1935 . P=21D.
              C 1936 .  HEOE KOEAH ECKA C OCTE-
              EHHM POCTOM CPEHEO ECKA OT 14.3M O 13.9M
              (1969) B CCTEME B. OTOEKTPECKE HAE-
              H B TEEHE 1968-69 . OKABAT KOEAH
              ECKA 12.33M-12.72M (V) C BOMOHM EPOAM
              15.4D B 1968  45.3D B 1969 . B 1973 . 12.28M-
              12.58MV, <B-V>=+1.37, P=50D 7101!./UNIQUE STAR.
              THE MEAN BRIGHTNESS INCREASED FROM 13.0M TO 12.4M
              SINCE 1889 TO 1915, AND FELL TO 12.8M IN 1926. FROM
              1895 TO 1926 REAL SHORTPERIODIC OSCILLATIONS WITH THE
              AMPLITUDE ABOUT 0.4M. IN 1928 THE AMPLITUDE SUDDENLY
              INCREASED BY ALMOST 2M, BUT THE MAGNITUDE IN MAXI-
              MUM REMAINED UNCHANGED. FROM 1928 TO 1935 THE LIGHT
              VARIATIONS BECAME PERIODIC, THE PERIOD INCREASING EVERY   R
YEA
              BY 1D IN ACCORDANCE WITH THE FORMULA: MIN=2426087+
              +15.933D*E+0.0233D*E**2. IN 1935 P=21D. SINCE
              1936 ONLY SMALL OSCILLATIONS OF BRIGHTNESS WITH A
              GRADUAL INCREASE OF THE MEAN MAGNITUDE FROM 14.3M TO
              13.9M B (1969). PHOTOELECTRIC OBSERVATIONS IN 1968-
              69 REVEAL THE LIGHT VARIATIONS 12.33M-12.72M V WITH
              POSSIBLE PERIODS 15.4D IN 1968 AND 45.3D IN 1969. IN
              1973 12.28M-12.58M V, <B-V>=+1.37, P=50D 7101!.
V727   SGR    VB A (B=V728 SGR, 14.7M-15.9M, 25", 108G).
V728   SGR    VB B (A=V727 SGR, B 25", 108G).
V734   SGR    MIN II 13.1.
V735   SGR    VB A (B 15.5M, 6", 315G). C O HAEHM B-V,
              U-B  CEKTP-HE OTHOCTC K T UG/ACCOR-
              DING TO B-V, U-B VALUES AND SPECTRUM THE STAR IS
              NOT A UG TYPE VARIABLE  9840!.
V738   SGR    B PAOHE APOBOO CKOEH/IN THE REGION OF THE
              GLOBULAR CLUSTER NGC 6558.
              COACHO/ACCORDING TO  5403!, RV? P=86.78D?
V743   SGR    MIN II 14.2.
V745   SGR    P VAR. MAX=2416560+385.1D*E (J.D.2411000-19260);
              OCE/SINCE J.D.2419260-CM.TA./SEE TABLE.
V748   SGR    MIN II 14.7; D=0.04P.
V750   SGR    D=0.02P:.
V752   SGR    MIN II 12.7.
V755   SGR    D=0.01P.
V757   SGR    MIN II 13.8; D=0.06P.
V760   SGR    MIN II 13.4. P VAR. MIN=2414059.5+45.10D*E (J.D.
              2412800-19000); OCE/SINCE J.D.2419000-CM.
              TA./SEE TABLE.
V761   SGR    MIN II 12.8; D=0.05P.
V762   SGR    P VAR. MAX=2414100+461D*E (J.D.2411000-22860);
              OCE/SINCE J.D.2422860-CM.TA./SEE TABLE.
V763   SGR    P VAR. EMEHT OBETBOPT HAEHM OC-
              E J.D.2415000./THE OBSERVATIONS ARE SATISFIED BY
              THE GIVEN ELEMENTS SINCE J.D.2415000.
V766   SGR    D=0.05P.
V768   SGR    MIN II 13.0.
V770   SGR    MIN II 13.1.
V773   SGR     A/H!=0.1.
V777   SGR    D=0.055P.
V778   SGR    MIN II 12.1.
V779   SGR    MIN II 12.0.
V780   SGR    MIN II 12.9; D=0.08P.
V782   SGR    D=0.045P.
V784   SGR    MIN II 12.8.
V786   SGR    D=0.025P.
V789   SGR    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER TR 31.
              P=5.10470D (MIN II 12.7)?  0478!.
V791   SGR    D=0.03P:.
V792   SGR    MIN II 12.2. B PAOHE PACCEHHOO CKOEH  -
              HO TMAHHOCT/IN THE REGION OF THE OPEN CLUSTER
              AND THE DIFFUSE NEBULA NGC 6514 (M 20).
V793   SGR    P VAR. MAX=2412610+195D*E (J.D.2412600-19400);
              OCE/SINCE J.D.2423400-CM.TA./SEE TABLE.
V794   SGR    P VAR. MIN I=2413723+173.48D*E (J.D.2413700-
              23750); OCE/SINCE J.D.2423750-CM.TA./SEE
              TABLE.
V801   SGR    MIN II 14.9.
V802   SGR     A/H!=-0.4.
V803   SGR    P=3.771748D?
V818   SGR    OPMA KPBO ECKA MEHETC./THE SHAPE OF THE
              LIGHT CURVE VARIES.
V819   SGR    P VAR?
V824   SGR    MIN II 15.2.
V828   SGR    K CTHK./THERE IS A CLOSE COMPANION.
V838   SGR    P VAR?
V839   SGR    P VAR? MAX=2426170.126+1.835347D*E (J.D.2425700-
              26600)  1598!; OCE/SINCE J.D.2441500-CM.TA./
              SEE TABLE.
V841   SGR    CM./SEE V818 SGR.
V844   SGR    P VAR?
V845   SGR    MIN II 14.6.
V859   SGR    CM./SEE V818 SGR.
V879   SGR    CM./SEE V828 SGR.
V882   SGR    MIN II 14.6.
V884   SGR    0.20P<=M-M<=0.40P. EKT AKO./BLAZHKO EFFECT.
V889   SGR    0.14P<=M-M<=0.24P. EKT AKO./BLAZHKO EFFECT.
V902   SGR    MIN II 14.8.
V903   SGR    MIN II 13.0.
V919   SGR    OCAHE CEKTPA/SPECTRUM DESCRIPTION  9845!.
V935   SGR    P VAR. MAX=2420040+232.0D*E (J.D.2419500-28650);
              OCE/SINCE J.D.2428600-CM.TA./SEE TABLE.
V938   SGR    P=138.27D?
V960   SGR    NP=1734D.
V966   SGR    MIN II 14.0.
V977   SGR    D=0.03P.
V981   SGR    MIN II 14.8.
V985   SGR    MIN II 14.3.
V986   SGR    D=0.015P.
V993   SGR    DI=0.05P:; MIN II 13.7, DII=0.09P, DII=0.00P.
V994   SGR    MIN II 12.8:.
V998   SGR    HA MIN II/THE DEPTH OF MIN II 0.04M:.
V1000  SGR    MIN II 13.9.
V1002  SGR    MIN II 13.7.
V1004  SGR     A/H!=-0.2.
V1005  SGR    MIN II 13.9.
V1013  SGR    MIN II 15.0.
V1017  SGR    VB B (A 10.6M V; B 15", 270G). OO CTAAC OB-
              TOPHO HOBO. HAAC TP HATEHE
              BCK: B 1901 (10.8M), 1919 (6.2M)  1973 (10.5M).
              CEKTP KOMHPOBAHH, CO CEAM OPEO
              KOMOHEHTA  3872!./FOR A LONG TIME THE STAR WAS
              CONSIDERED TO BE A RECURRENT NOVA. THREE CONSIDERABLE
              FLARES WERE OBSERVED: IN 1901 (10.8M), 1919 (6.2M),
              AND 1973 (10.5M). COMPOSITE SPECTRUM WITH A TRACE
              OF A HOT COMPONENT  3872!.
V1023  SGR    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER CR 394. MIN II 13.0:.
V1026  SGR    MIN II 13.4.
V1028  SGR    MIN II 14.4.
V1032  SGR    MIN II 15.0.
V1033  SGR    CM./SEE V818 SGR. EKT AKO?/BLAZHKO
              EFFECT?
V1034  SGR    D=0.025P:.
V1049  SGR    MIN II 13.6; MIN II-MIN I=0.326P; DII=0.025P.
V1050  SGR    MIN II 14.1.
V1056  SGR    MIN II 14.1.
V1063  SGR    OPMA KPBO ECKA CHO MEHETC. EKT
              AKO?/THE SHAPE OF THE LIGHT CURVE STRONGLY VARI-
              ES. BLAZHKO EFFECT?
V1068  SGR    MIN II 15.4.
V1069  SGR    CM./SEE V1063 SGR.
V1071  SGR    P=1.3560996D?
V1072  SGR    CM./SEE V1063 SGR.
V1080  SGR    P VAR. CM./SEE V818 SGR.
V1081  SGR    P VAR?
V1089  SGR    K/CYCLE<=30D.
V1100  SGR    D=0.02P:.
V1108  SGR    MIN II 11.9; MIN II-MIN I=0.516P.
V1109  SGR    MIN II 14.5.
V1127  SGR    EMEHT COEPAT KBAPATH EH:/THERE IS A
              NONLINEAR TERM IN THE ELEMENTS:+78.10D**-10*E**2.
V1136  SGR    D=0.020P.
V1148  SGR    B PAOHE APOBOO CKOEH/IN THE REGION OF THE
              GLOBULAR CLUSTER NGC 6553.
V1153  SGR    P VAR? MAX=2428391.266+1.332624D*E (J.D.2427680-
              30910); OCE/SINCE J.D.2435630-CM.TA./SEE
              TABLE.
V1177  SGR    MIN II 11.4.
V1178  SGR    D=0.03P:.
V1180  SGR     A/H!=-0.4.
V1181  SGR     A/H!=0.6. P VAR. MAX=2428452.25+21.341D*E (J.D.
              2427400-31000)  1638!; OCE/SINCE J.D.2433000-
              CM.TA./SEE TABLE.
V1185  SGR     A/H!=-0.5. P VAR. MAX=2428778.86+13.9123D*E
              (J.D.2427500-32750)  1638!; MAX=2437485.4+
              +13.901345D*E (J.D.2437100-43760)  8519!; OCE/
              SINCE J.D.2444000-CM.TA./SEE TABLE.
V1187  SGR     A/H!=-0.8.
V1188  SGR     CA/H!=-0.37.
V1189  SGR     A/H!=-1.1.
V1190  SGR    P=3.000078D?
V1191  SGR    MIN II 14.4.
V1205  SGR    BOMOEH COPEHH EPO:/THE ALTERNATIVE
              PERIOD IS POSSIBLE: 0.659820D  1638!.
V1209  SGR    A VAR.
V1211  SGR    DS=3:.
V1214  SGR    EMEHT COEPAT KBAPATH EH:/THERE IS A
              NONLINEAR TERM IN THE ELEMENTS:-0.25D*10**-7*E**2.
V1216  SGR    MU=0.720", P=106.7G.
V1223  SGR    KAK PABO, HAXOTC B BOEHHOM COCTOH;
              OTMEEH T AEH ECKA HA HECKOKO BE-
              H  BEHAATETH HTEPBA HEPABHX -
              MEHEH P POMETOHX BEHAX./AS A RULE
              HAS A PERSISTENT HIGH STATE; FIVE DROPS BY TWO TO MORE
              THAN THREE MAGNITUDES HAVE BEEN REGISTERED AND A
              TWELVE YEAR INTERVAL OF IRREGULAR VARIATIONS AT INTER-
              MEDIATE MAGNITUDES.
              COACHO  9850!, HAATC MEEHHE MEHE-
              H ECKA HA 0.15M A 1D. HA HX HAKABATC
              KOEAH C EPOOM OPTAHOO BEH PORB
              (MAX=2444749.9866+0.140239D*E)  AMTO
              O 0.15M. HA T KOEAH HAKABATC PE:
              C P=794.38S  AMTO OT 0.03M O 0.15M (MAX=
              =2444750.00404+0.009194215D*E)  (HOA) C
              P=849.8S C BBOE MEHE AMTO (MAX=
              =2444750.00350+0.00983588D*E). KPOME TOO, HA-
              ATC CTPE MEHEH ECKA HA 0.10M-
              0.20M A 10-100S  BCOKOACTOTHE MEPAH HA
              0.05M. COACHO  9851!, EPO PEHTEHOBCKX M-
              COB, OTOECTBEM C EPOOM BPAEH
              KOMAKTHOO O'EKTA, PABEH 12.5 MH./ACCORDING
              TO  9850! THERE ARE SLOW VARIATIONS IN BRIGHTNESS BY
              0.15M ON A TIME SCALE OF-1 DAY. THEY ARE SUPERIMPO-
              SED BY VARIATIONS WITH THE ORBITAL PERIOD PORB (MAX=
              =2444749.9866+0.140239D*E) AND WITH AMPLITUDE UP
              TO 0.15M. THESE VARIATIONS IN THEIR TURN ARE SUPERIMPO-
              SED BY THE OTHERS: WITH P=794.38S AND THE AMPLITUDE
              FROM 0.03M UP TO 0.15M (MAX=2444750.00404+
              +0.009194215D*E AND (SOMETIMES) WITH P=849.8S AND
              A TWICE SMALLER AMPLITUDE (MAX=2444750.00350+
              +0.00983588D*E). BESIDES THERE ARE RAPID BRIGHTNESS
              VARIATIONS ON TIME SCALES 10-100S BY 0.10M-0.20M,
              AND HIGH FREQUENCY FLICKERING BY 0.05M. ACCORDING TO
               9851!, THE PERIOD OF X-RAY PULSES ASSOCIATED WITH
              THE ROTATION OF THE COMPACT OBJECT IS 12.5 MINUTES.
V1276  SGR    MIN II 14.3.
V1280  SGR    BEHA B MAX MEHETC HA 2M C EPOOM 5230D./
              BRIGHTNESS OF MAX VARIES BY 2M WITH THE PERIOD
              5230D.
V1281  SGR    MEHEHE ECKA HE CTPOO EPOHO./THE LIGHT
              VARIATION IS NOT STRICTLY PERIODIC.
V1282  SGR    P VAR. MIN=2427651.297+1.754574D*E (J.D.2427650-
              30560)  0705!; OCE/SINCE J.D.2435600-CM.TA./
              SEE TABLE.
V1284  SGR    MIN II 13.5. EB?
V1287  SGR    CM./SEE V703 SGR.
              VAR 3. COACHO  2951!, PEE MEHEH ECKA,
              T EPEMEHHOCT  EMEHT MEHEH ECKA B
               1640! OOHO PCAH BEE VAR 4./ACCOR-
              DING TO  2951! THE RANGE OF LIGHT VARIATION, THE TYPE
              OF VARIABILITY AND THE ELEMENTS OF LIGHT VARIATION ARE
              ERRONEOUSLY ASSIGNED IN  1640! TO THE STAR VAR 4.
              MIN II 14.8.
V1290  SGR     A/H!=-1.2.
V1303  SGR     A/H!=-0.8. P VAR? MAX=2438241.176+18.46812D*E
              (J.D.2427700-38250)  0001!; OCE/SINCE J.D.
              2444000-CM.TA./SEE TABLE.
V1304  SGR     A/H!=0.3. P VAR. MAX=2428758.10+12.9287D*E
              (J.D.2427590-28820)  1640!; OCE/SINCE J.D.
              2435600-CM.TA./SEE TABLE.
V1309  SGR    HEAEKO OT V4032 SGR./NOT FAR FROM V4032 SGR.
V1311  SGR    V14 B APOBOM CKOEH/V 14 IN THE GLOBULAR CLUS-
              TER NGC 6656 (M22).
              HE EH CKOEH./NOT A MEMBER OF THE CLUSTER.
V1312  SGR    P VAR? MAX=2428815.600+0.6011427D*E (J.D.
              2427590-28820)  1640!; OCE/SINCE J.D.2435630-
              CM.TA./SEE TABLE.
V1314  SGR    P VAR? MAX=2428346.536+0.657489D*E (J.D.2427600-
              28820)  1640!; OCE/SINCE J.D.2435630-CM.TA./
              SEE TABLE.
V1317  SGR    P VAR?
V1327  SGR    SR?, L?  8424!.
V1328  SGR    P=0.39937D?
V1329  SGR    VB B (A 17.2M; B 1.4", 120G). P VAR. MAX=2432388.777+
              +0.48306D*E (J.D.2431670-32740)  3524!; OCE/
              SINCE J.D.2443300-CM.TA./SEE TABLE.
V1331  SGR    MIN II 16.5.
V1352  SGR    P VAR. MAX=2431998.851+0.49505D*E (J.D.2431670-
              33150)  1680!; MAX=2443341.844+0.49493D*E (J.D.
              2443300-350); MAX=2444087.558+0.49516D*E (J.D.
              2444050-110); B HTEPBAE/IN THE INTERVAL J.D.
              2444400-410-CM.TA./SEE TABLE.
V1356  SGR    MIN II 18.0:.
V1357  SGR    MIN II 19.0.
V1359  SGR    P VAR?
V1369  SGR    P VAR. MAX=2432736.821+0.52956D*E (J.D.2431670-
              33150)  3524!; OCE/SINCE J.D.2440700-CM.TA./
              SEE TABLE.
V1374  SGR    DS=1.
V1378  SGR    DS=-3:.
V1387  SGR    DS=3.
V1389  SGR    AHA OXA MIN ECKA./THE EPOCH OF MIN BRIGHTNESS
              IS GIVEN.
V1390  SGR    MIN II 17.6.
V1392  SGR    P VAR. MAX=2432739.791+0.55032D*E (J.D.2431670-
              33150)  3524!; OCE/SINCE J.D.2440700-CM.TA./
              SEE TABLE.
V1393  SGR    DS=3.
V1394  SGR    MIN II 18.0.
V1401  SGR    CM./SEE V1389 SGR.
V1405  SGR    P VAR. MAX=2432031.778+0.46511D*E (J.D.2431670-
              33150)  6094!; OCE/SINCE J.D.2443300-CM.TA./
              SEE TABLE.
V1408  SGR    A VAR (0.5M<=A<=1.4M).
V1409  SGR    P VAR. MAX=2432739.822+0.65159D*E (J.D.2431670-
              33150)  3524!; OCE/SINCE J.D.2443300-CM.TA./
              SEE TABLE.
V1412  SGR    CM./SEE V1389 SGR.
V1415  SGR    P VAR?
V1416  SGR    DS=3. P VAR? MAX=2432002.875+0.42767D*E
              (J.D.2431670-33150)  6094!; OCE/SINCE J.D.
              2440700-CM.TA./SEE TABLE.
V1418  SGR    P VAR. MAX=2432740.818+0.45423D*E (J.D.2431670-
              33150)  3524!; OCE/SINCE J.D.2440700-CM.TA./
              SEE TABLE.
V1419  SGR    P VAR. MAX=2432061.669+0.57144D*E (J.D.2431670-
              33150)  1680!; OCE/SINCE J.D.2440700-CM.TA./
              SEE TABLE.
V1425  SGR    MIN II 18.8.
V1426  SGR    DS=1.5.
V1429  SGR    CM./SEE V1389 SGR.
V1435  SGR    MIN II 18.0; MIN II-MIN I=0.53P.
V1437  SGR    V8 (NGC 6522); HE EH APOBOO CKOEH/NOT A
              MEMBER OF THE GLOBULAR CLUSTER.
V1438  SGR    V9 (NGC 6522); HE EH APOBOO CKOEH/NOT A
              MEMBER OF THE GLOBULAR CLUSTER.
V1439  SGR    P=0.53711D?  6094!.
V1443  SGR    MIN II 18.6.
V1446  SGR    MIN II 18.0.
V1447  SGR    MIN II 18.2.
V1454  SGR    MIN II 15.4.
V1457  SGR    MIN II 19.0.
V1459  SGR    HA MIN II/THE DEPTH OF MIN II IS 0.04M.
V1460  SGR    P VAR. MAX=2432067+162.0D*E (J.D.2431670-33150)
               1680!; OCE/SINCE J.D.2440340-CM.TA./SEE
              TABLE.
V1464  SGR    DS=1.
V1465  SGR    P VAR. MAX=2431702.660+0.45757D*E (J.D.2431700-
              940); MAX=2432706.945+0.45757D*E (J.D.2431940-
              32740)  3524!; OCE/SINCE J.D.2440740-CM.TA./
              SEE TABLE.
V1466  SGR    CM./SEE V1389 SGR.
V1473  SGR    COACHO/ACCORDING TO  8424!, P=340D.
V1487  SGR    MIN II 18.8.
V1491  SGR    MIN II 18.5.
V1498  SGR    SP KOMOHEHT TECHO AP./SP COMPONENT OF A CLOSE
              PAIR. P VAR. MAX=2432739.728+0.47467D*E
              (J.D.2431670-33150)  6094!; OCE/SINCE J.D.
              2443300-CM.TA./SEE TABLE.
V1508  SGR    VB.
V1509  SGR    MIN II 18.1:.
V1510  SGR    COACHO/ACCORDING TO  6094!, P=0.48546D.
V1516  SGR    P VAR? MAX=2432740.753+0.49709D*E (J.D.2431670-
              33150)  3524!; OCE/SINCE J.D.2440700-CM.TA./
              SEE TABLE.
V1517  SGR    P<2.0D.
V1523  SGR    P VAR? MAX=2432417.702+0.36202D*E (J.D.2431670-
              33150)  3524!; OCE/SINCE J.D.2443300-CM.TA./
              SEE TABLE.
V1526  SGR    MIN II 18.3.
V1537  SGR    MIN II 17.4; MIN II-MIN I=0.54P.
V1540  SGR    COACHO/ACCORDING TO  8424!, P=465D.
V1546  SGR    CM./SEE V1389 SGR.
V1550  SGR    P=0.37432D?  6094!.
V1554  SGR    MIN II 17.5.
V1557  SGR    DS=8.
V1558  SGR    DS=1.
V1559  SGR    CM./SEE V1459 SGR.
V1561  SGR    MIN II 17.7.
V1567  SGR    MIN II 18.0.
V1569  SGR    MIN II 18.6.
V1576  SGR     CA/H!=-1.23.
V1577  SGR    P VAR. MAX=2426200+290D*E (J.D.2426000-30560)
               2449!; OCE/SINCE J.D.2430560-CM.TA./SEE
              TABLE.
V1580  SGR    P VAR (310D<=P<=365D).
V1589  SGR     CA/H!=-0.91.
V1602  SGR    D=0.03P.
V1610  SGR    P<0.5D.
V1639  SGR    CM./SEE V818 SGR.
V1640  SGR    (K-B)2=0.24. P VAR?
V1642  SGR    250D<=P<=350D.
V1643  SGR    MIN II 12.1. COACHO/ACCORDING TO  5771!, RR?, P=
              =0.34D.
V1644  SGR    CM./SEE V818 SGR.
V1647  SGR    VB A (B 9.13M, 8", 104G). MIN II 7.43, DII=0.059P,
              MIN II-MIN I=0.262P (J.D.2441830); MIN II=
              =2441830.55561+3.28282227D*E.
              EPO BPAEH H AC 592.5+-6.5 OA./THE
              APSIDAL MOTION PERIOD IS 592.5+-6.5 YEARS.
V1648  SGR    TECHA VB. OCK MIN./CLOSE VB. FLAT MIN.
V1652  SGR    CM./SEE V1648 SGR.
V1653  SGR    CM./SEE V1648 SGR.
V1656  SGR    CM./SEE V1648 SGR.
V1658  SGR    P VAR.MAX=2426560+105D*E (J.D.2417000-28000)
               0842!; OCE/SINCE J.D.2428000-CM.TA./SEE
              TABLE.
V1660  SGR    CM./SEE V1648 SGR.
V1661  SGR    CM./SEE V1648 SGR.
              P VAR. MAX=2426850+275D*E (J.D.2424000-26850);
              OCE/SINCE J.D.2436700-CM.TA./SEE TABLE.
V1667  SGR    P VAR. MAX=2426560+158D*E (J.D.2417000-36000)
               0842!; OCE/SINCE J.D.2436000-CM.TA./SEE
              TABLE.
V1668  SGR    CM./SEE V1648 SGR.
V1670  SGR    A VAR. P VAR. OPMA KPBO ECKA MEHETC (BO-
              MOHO, C EPOOM OKOO 11 ET)./THE SHAPE OF THE
              LIGHT CURVE VARIES (PROBABLY WITH A PERIOD OF ABOUT
              11 YEARS).
V1675  SGR    BOMOH CTHK 16M./A POSSIBLE COMPANION OF
              16M.
V1679  SGR    CM./SEE V1648 SGR.
V1681  SGR    CM./SEE V1675 SGR.
V1690  SGR    CM./SEE V1675 SGR.
V1691  SGR    CM./SEE V1648 SGR.
              P VAR. MAX=2426520+235D*E (J.D.2417000-28000)
               0842!; OCE/SINCE J.D.2436000-CM.TA./SEE
              TABLE.
V1697  SGR    CM./SEE V1675 SGR.
V1698  SGR    CM./SEE V1675 SGR.
V1699  SGR    P VAR. MAX=2425410+203.6D*E (J.D.2417000-27600)
               0842!; OCE/SINCE J.D.2436000-CM.TA./SEE
              TABLE.
V1703  SGR    CM./SEE V1675 SGR.
V1705  SGR    P VAR. MAX=2425860+142D*E (J.D.2417000-27000)
               0842!; OCE/SINCE J.D.2435800-CM.TA./SEE
              TABLE.
V1711  SGR     A/H!=-1.1. P VAR. MAX=2435365.19+30.46D*E
              (J.D.2432700-35400)  2570!; OCE/SINCE J.D.
              2442200-CM.TA./SEE TABLE.
V1714  SGR    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER RUPRECHT 134.
V1721  SGR    D=0.03P:.
V1723  SGR    MIN II 13.8.
V1730  SGR    MIN II 14.8:; D=0.03P:.
V1741  SGR    B TMAHHOCT  CKOEH/IN THE NEBULA AND THE
              CLUSTER NGC 6530 (M8). VAR1.
V1743  SGR    CM./SEE V1741 SGR. VAR 2.
V1747  SGR    CM./SEE V1741 SGR. VAR 3.
V1748  SGR    CM./SEE V1741 SGR. VAR 4.
V1749  SGR    CM./SEE V1741 SGR. VAR 6.
V1750  SGR    CM./SEE V1741 SGR. VAR 8.
V1751  SGR    CM./SEE V1741 SGR. VAR 7.
V1752  SGR    CM./SEE V1741 SGR. VAR 13.
V1753  SGR    CM./SEE V1741 SGR. VAR 14.
V1755  SGR    CM./SEE V1741 SGR. VAR 15.
V1758  SGR    CM./SEE V1741 SGR. VAR 16.
V1761  SGR    CM./SEE V1741 SGR. VAR 19.
V1762  SGR    CM./SEE V1741 SGR. VAR 20.
V1764  SGR    CM./SEE V1741 SGR. VAR 23.
V1765  SGR    CM./SEE V1741 SGR. VAR 24.
V1768  SGR    CM./SEE V1741 SGR. VAR 26.
V1769  SGR    CM./SEE V1741 SGR. VAR 27.
V1771  SGR    CM./SEE V1741 SGR. VAR 29.
V1772  SGR    CM./SEE V1741 SGR. VAR 28.
V1773  SGR    CM./SEE V1741 SGR. VAR 31.
V1774  SGR    CM./SEE V1741 SGR. VAR 30.
V1775  SGR    CM./SEE V1741 SGR. VAR 33.
V1776  SGR    CM./SEE V1741 SGR. VAR 36.
V1777  SGR    CM./SEE V1741 SGR. VAR 37.
V1778  SGR    CM./SEE V1741 SGR. VAR 34.
V1779  SGR    CM./SEE V1741 SGR. VAR 40.
V1780  SGR    CM./SEE V1741 SGR. VAR 39.
V1781  SGR    CM./SEE V1741 SGR. VAR 41.
V1782  SGR    CM./SEE V1741 SGR. VAR 44.
V1784  SGR    CM./SEE V1741 SGR. VAR 45.
V1785  SGR    CM./SEE V1741 SGR. VAR 46.
V1786  SGR    CM./SEE V1741 SGR. VAR 48.
V1787  SGR    CM./SEE V1741 SGR. VAR 47.
V1788  SGR    CM./SEE V1741 SGR. VAR 50.
V1789  SGR    CM./SEE V1741 SGR. VAR 51.
V1790  SGR    CM./SEE V1741 SGR. VAR 49. AAH KOMOHEHT
              TECHO BOHO/WESTERN COMPONENT OF A CLOSE PAIR.
V1791  SGR    CM./SEE V1741 SGR. VAR 53.
V1792  SGR    CM./SEE V1741 SGR. VAR 55.
V1793  SGR    CM./SEE V1741 SGR. VAR 54.
V1794  SGR    CM./SEE V1741 SGR. VAR 56.
V1795  SGR    CM./SEE V1741 SGR. VAR 58.
V1797  SGR    CM./SEE V1741 SGR. VAR 59.
V1798  SGR    CM./SEE V1741 SGR. VAR 60.
V1800  SGR    CM./SEE V1741 SGR. VAR 61.
V1801  SGR    CM./SEE V1741 SGR. VAR 62.
V1802  SGR    CM./SEE V1741 SGR. VAR 63.
V1803  SGR    CM./SEE V1741 SGR. VAR 64. SP KOMOHEHT TECHO
              BOHO./SP COMPONENT OF A CLOSE PAIR.
V1805  SGR    CM./SEE V1741 SGR. VAR 66.
V1807  SGR    CM./SEE V1741 SGR. VAR 67.
V1808  SGR    CM./SEE V1741 SGR. VAR 68.
V1828  SGR    P VAR. MAX=2424402+12.985D*E (J.D.2423800-
              36000)  2515!; OCE/SINCE J.D.2436000-CM.TA./
              SEE TABLE.
V1831  SGR    P VAR. MAX=2428849.4+26.58D*E (J.D.2427500-
              31270)  2447!; OCE/SINCE J.D.2435630-CM.TA./
              SEE TABLE.
V1843  SGR    P=163.7D?  5869!.
V1845  SGR    OCK MIN. TECH CTHK?/FLAT MIN. CLOSE
              COMPANION?
V1864  SGR    PBEEHA OXA MAX ECKA./EPOCH OF LIGHT MAXI-
              MUM IS GIVEN.
V1869  SGR    P VAR. MAX=2434178+346D*E (J.D.2427590-34220)
               2447!; OCE/SINCE J.D.2435630-CM.TA./SEE
              TABLE.
V1882  SGR    CM./SEE V818 SGR.
V1891  SGR    CTHK 16M./A COMPANION OF 16M.
V1894  SGR    V4 (NGC 6637). BOMOH EH APOBOO CKOE-
              H/POSSIBLE MEMBER OF THE GLOBULAR CLUSTER NGC
              6637 (M 69).
V1895  SGR    P VAR. MAX=2421065+156.0D*E (J.D.2418850-21100);
              OCE/SINCE J.D.2427600-CM.TA./SEE TABLE.
V1900  SGR    CTHK 15M./A COMPANION OF 15M.
V1904  SGR    CM./SEE V1900 SGR.
V1911  SGR    P VAR. MAX=2428832.4+10.0581D*E (J.D.2427600-
              34220)  2447!; OCE/SINCE J.D.2435630-CM.TA./
              SEE TABLE.
              OPMA KPBO ECKA MEHETC?/THE SHAPE OF THE
              LIGHT CURVE VARIES?
V1925  SGR    P VAR?
V1942  SGR    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER RUPRECHT 147.
V1945  SGR    CM./SEE AU SGR.
V1946  SGR    CM./SEE AU SGR.
V1947  SGR    CM./SEE AU SGR. BCE OKOBAHHE KAPT OKPE-
              CTHOCTE TO EPEMEHHO HEPABH. COACHO
               9861!, EPEMEHHA PACOOEHA HA 1.1 MM K 
               HA 0.8 MM K BOCTOK OT BE D2, OTMEEHHO
              HA PC.3 B CTATE  2428!./ALL THE PUBLISHED CHARTS
              FOR THIS VARIABLE ARE WRONG. ACCORDING TO  9861! THE
              STAR ACTUALLY LIES 1.1 MM SOUTH AND 0.8 MM EAST OF
              "D2" IN FUGURE 3 PUBLISHED IN  2428!.
V1948- V1951  SGR CM./SEE AU SGR.
V1954  SGR    VB(RO=2"). P VAR. EMEHT COEPAT KBAPATH
              EH:/THERE IS A NONLINEAR TERM IN THE ELEMENTS:
              -4.1313D*10**-8*E**2.
V1958  SGR    MIN II 14.0.
V1962  SGR    B PAOHE PACCEHHOO CKOEH  HO T-
              MAHHOCT/IN THE REGION OF THE OPEN CLUSTER AND THE
              DIFFUSE NEBULA NGC 6618 (M 17).
V1963  SGR    CM./SEE V1962 SGR.
V1966  SGR    CM./SEE V1962 SGR.
V1969  SGR    TP TECHX CAX CTHKA (15.8M-16.3M)./THERE
              ARE THREE CLOSE FAINT COMPANIONS (15.8M-16.3M).
V1970  SGR    CM./SEE V1962 SGR.
V1971  SGR    CM./SEE V1962 SGR.
V1973  SGR    CM./SEE V1962 SGR.
V1975  SGR    CM./SEE V1962 SGR. BOMOHO HAE OOO
              CTHKA./THE PRESENCE OF A BLUE COMPANION IS POS-
              SIBLE.
V1976- V1977  SGR CM./SEE V1962 SGR.
V1980  SGR    MIN II 11.7; DII=0.11P; MIN II-MIN I=0.52P.
V1996  SGR    VB.
V2003  SGR    S 5.5/5. CM./SEE Y SGR.
V2007  SGR    V 26 (NGC 6656=M 22).
V2008  SGR    P=120-135D.
V2028  SGR    B PAOHE APOBOO CKOEH/IN THE REGION OF THE
              GLOBULAR CLUSTER NGC 6681 (M 70).
V2037  SGR    BOMOEH TECH CTHK./A CLOSE COMPANION IS
              POSSIBLE.
V2054  SGR    P>450D?
V2064  SGR    VB. OEHBAC CMMAPH ECK BE  KO-
              O KOMOHEHTA. HE CHO, KAKA  HX MEHETC./
              COMBINED BRIGHTNESS OF THE STAR AND THE CLOSE COMPA-
              NION WAS ESTIMATED. IT IS NOT CLEAR WHICH STAR IS VARI-
              ABLE.
V2065  SGR    NP KOMOHEHT TECHO BOHO/NP COMPONENT OF A CLO-
              SE BINARY.
V2094  SGR    P<0.5D.
V2106  SGR    VB. OEHBAC CMMAPH ECK KOMOHEHTOB./
              COMBINED BRIGHTNESS OF THE COMPONENTS WAS ESTIMA-
              TED.
V2148  SGR    CM./SEE V2106 SGR.
              EPEMEHHA-CEBEPH KOMOHEHT./THE VARIABLE
              IS THE NORTHERN COMPONENT.
V2276  SGR    P<30D.
V2282  SGR    BEA/STAR L. CM./SEE V1945 SGR. CEKTP-O-
              H./LATE SPECTRUM.
V2283  SGR    MIN II 10.59:. BPAEHE H AC C P=560 ET/
              APSIDAL MOTION WITH P=560 YEARS  7107!:
              0.739P (1898)<=MIN II-MIN I<=0.797P (1965).
              EMEHT, PBEEHHE B TAE, COEPAT CH-
              COAHE EH:/THERE ARE PERIODIC TERMS IN THE
              ELEMENTS GIVEN IN THE TABLE:
              +0.5414D SIN 0.006G (E+45019)-0.0995D SIN 0.012G*
              (E+45019)+0.0217D SIN 0.018G (E+45019); MIN II=
              =2438946.7619+3.4714231D*E-0.5414D SIN 0.006G*
              (E+45019)-0.0995D SIN 0.012G (E+45019)-0.0217D*
              SIN 0.018G (E+45019).
V2284  SGR    P VAR.
V2285  SGR    B PAOHE APOBOO CKOEH/IN THE REGION OF THE
              GLOBULAR CLUSTER NGC 6558.
V2313  SGR    MIN II 16.8.
V2315  SGR    P=0.193D?
V2323  SGR    OA/BLUE  8424!.
V2341  SGR    CM./SEE V1389 SGR.
V2342  SGR    V 17 (NGC 6626=M28). EH TOO APOBOO CKOE-
              H./THE MEMBER OF THIS GLOBULAR CLUSTER. MIN II 13.5.
V2343  SGR    K CTHK 14.5M./A CLOSE COMPANION OF 14.5M.
V2346  SGR    K/CYCLES 50-100D.
V2349  SGR    MIN II 9.2.
V2351  SGR    MIN II 10.31.
V2352  SGR    P VAR. EMEHT COEPAT KBAPATH EH:/
              THERE IS A NONLINEAR TERM IN THE ELEMENTS:
              +0.0525D*E**2.
V2355  SGR    B PAOHE APOBOO CKOEH/IN THE REGION OF THE
              GLOBULAR CLUSTER NGC 6637 (M 69).
V2358  SGR    B PAOHE APOBOO CKOEH/IN THE REGION OF THE
              GLOBULAR CLUSTER NGC 6642.
V2359- V2361  SGR CM./SEE V2355 SGR.
V2362  SGR    K CTHK 15M./A CLOSE COMPANION OF 15M.
V2366  SGR    P VAR. EMEHT COEPAT KBAPATH EH:/
              THERE IS A NONLINEAR TERM IN THE ELEMENTS:
              +0.6815D*10**-9*E**2.
V2367  SGR    V28 (NGC 6656=M22). HE EH TOO APOBOO
              CKOEH./NOT A MEMBER OF THIS GLOBULAR CLUSTER.
              P=323D?
V2378  SGR    BA KX CTHKA 15.3M  15.8M./TWO CLOSE
              COMPANIONS OF 15.3M AND 15.8M.
V2389  SGR    P VAR?
V2391  SGR    P=189D?
V2413  SGR    P VAR. EMEHT CPABEB B HTEPBAE/THE ELE-
              MENTS ARE VALID IN THE INTERVAL J.D.2425440-30905.
V2416  SGR    P.K. 7+1G2.
V2425  SGR    E?
V2442  SGR    P=0.5D?
V2449  SGR    MIN II 17.4.
V2468  SGR    CM./SEE V2323 SGR.
V2471  SGR    VB B (A 14.6M; B 8", 225G).
V2493  SGR    CM./SEE V2323 SGR.
V2506  SGR    P.K. 3-4G6.
V2507  SGR    MIN II 14.6.
V2508  SGR    MIN II 14.1:.
V2509  SGR    MIN II 7.50.
V2510  SGR    CM./SEE V1389 SGR.
              P VAR. EMEHT, PBEEHHE B TAE, OBET-
              BOPT HAEHM OCE J.D.2427440./THE ELE-
              MENTS GIVEN IN THE TABLE ARE VALID SINCE J.D.
              2427440.
V2520  SGR    VB.
V2526  SGR    CM./SEE V1389 SGR.
              P VAR. MIN=2428699.5+31.3224D*E (J.D.2424100-
              31400)  5590!. OCE/SINCE J.D.2431400-CM.TA./
              SEE TABLE.
V2529  SGR    MIN II 14.5. B  5590! PBEEH OOBHH EPO./
              TWICE SHORTER PERIOD IS GIVEN IN  5590!.
V2540  SGR    P VAR.
V2544  SGR    VB?
V2552  SGR    VB A (B 15.7M).
V2553  SGR    BA KX CTHKA./THERE ARE TWO CLOSE COMPA-
              NIONS.
V2562  SGR    CEBEPH KOMOHEHT TECHO AP. CTHK 16M./
              NORTHERN COMPONENT OF A CLOSE PAIR. THE COMPANION
              IS OF 16M.
V2563  SGR    P VAR.
V2564  SGR    P VAR?
V2565  SGR    VB B (A 12.5M; B 90G).
V2566  SGR    P VAR.  CA/H!=-0.52.
V2567  SGR     CA/H!=-0.57.
V2568  SGR    P VAR?
V2576  SGR    P VAR. MAX=2426200+149D*E (J.D.2423500-27000);
              OCE/SINCE J.D.2433000-CM.TA./SEE TABLE.
V2577  SGR    P VAR?
V2578  SGR    VB. CM./SEE V2358 SGR.
V2579  SGR    P VAR. MAX=2429926.251+0.5911903D*E (J.D.2427590-
              34200)  5590!; OCE/SINCE J.D.2435600-CM.TA./
              SEE TABLE.
V2584  SGR    P VAR. MAX=2426564.347+0.534829D*E (J.D.2423940-
              33860); OCE/SINCE J.D.2437820-CM.TA./SEE
              TABLE.
V2592  SGR    B PAOHE APOBOO CKOEH/IN THE REGION OF THE
              GLOBULAR CLUSTER NGC 6656 (M22).
V2593  SGR    P VAR. MAX=2428780.349+0.5123825D*E (J.D.
              2427680-34200)  5590!; OCE/SINCE J.D.2435600-
              CM.TA./SEE TABLE.
V2594  SGR    P VAR.
V2598  SGR    CTHK/A COMPANION 15.8M.
V2601  SGR    P.K. 12-7G1. CM./SEE V1389 SGR.
              OCAHE CEKTPA/SPECTRUM DESCRIPTION  6495!.
V2610  SGR    P VAR.
V2616  SGR    MIN II 13.0.
V2617  SGR    MIN II 9.63.
V2620  SGR    P=185.6D?
V2625  SGR    P=0.75837D?
V2628  SGR    P=171D:?/205D:?/256D:?.
V2645  SGR    P VAR?
V2649  SGR    P=143D:?
V2672  SGR    P=196.8D?/204.5D, /255.3D?/315.0D?
V2682  SGR    P=228.5D?
V2687  SGR    P=174D:?
V2703  SGR    P=270D:?
V2719  SGR    SR?
V2731  SGR    P=147D:?
V2732  SGR    P=188.6D?
V2733  SGR    P=244D:?
V2736  SGR     CA/H!=-1.45.
V2738  SGR     CA/H!=-0.67.
V2740  SGR    P=269.0D?
V2745  SGR     CA/H!=-1.15.
V2756  SGR    P.K. 2-5G1. CM./SEE V1389 SGR.
V2763  SGR    P=216D:?
V2777  SGR     CA/H!=-0.83.
V2783  SGR    P=265.0D?
V2789  SGR    P=255.5D?
V2798  SGR    P=244.5D?
V2816  SGR    P=250D:?
V2828  SGR    P=0.39669D?
V2830  SGR    EEA?/CEPHEID?
V2833  SGR    P=224.0D?
V2834  SGR    P=275D:?
V2846  SGR    P=0.39659D?
V2868  SGR    P=235.5D?
V2876  SGR    MIN II 15.7:.
V2877  SGR    P=254.5D?
V2893  SGR    P=250D:?
V2900  SGR    P=0.49835D?
V2905  SGR    OCAHE CEKTPA/SPECTRUM DESCRIPTION  4452,
              6495!.
V2918  SGR    P=197D:?
V2937  SGR     CA/H!=-0.75.
V2947  SGR    RV TAU? EEA?/CEPHEID?
V2959  SGR    P=0.37233D?
V2962  SGR    P=209.5D?
V2967  SGR    P=0.68750D?
V2988  SGR    P=213.0D? CM./SEE V3033 SGR.
V2996  SGR    CM./SEE V2947 SGR.
V3004  SGR     CA/H!=-0.76.
V3005  SGR    CM./SEE V2947 SGR.
V3016  SGR    P VAR?
V3032  SGR    P=153D:?
V3033  SGR    KOOPHAT, AHHE B  5869!, OOH./THE CO-OR-
              DINATES GIVEN IN  5869! ARE ERRONEOUS.
V3034  SGR    P=154D:?
V3038  SGR    P=252D:?
V3052  SGR    CM./SEE V2947 SGR.
V3062  SGR    EW? P=0.59610D?
V3065  SGR    P=179.8D?/215.5D?
V3071  SGR    P=291D:?
V3072  SGR    P=194D:?
V3088  SGR    P=215D:?
V3105  SGR     CA/H!=-0.82.
V3106  SGR    P=261D:?
V3111  SGR    P=182.8D?
V3127  SGR    UG? HE KPACHA./NOT RED.
V3128  SGR    NOVA? HAAC TOKO OH MAX./ONLY ONE MAX
              WAS OBSERVED.
V3170  SGR     CA/H!=-0.82.
V3175  SGR    P=179.8D?
V3176  SGR    P=197D:?
V3179  SGR    P=297D:?
V3186  SGR     CA/H!=-1.28.
V3190  SGR    P=227.0D?
V3196  SGR    CM./SEE V2947 SGR.
V3207  SGR    P=237D:?
V3239  SGR    P=226D:?
V3249  SGR    UG?
V3285  SGR    P=173.8D/196.2D?
V3294  SGR    P=121D:?/177D:?
V3295  SGR    P=197D:?
V3335  SGR    CM./SEE V2947 SGR.
V3353  SGR    P VAR?
V3356  SGR    P=239.5D?
V3365  SGR    P=197D:?/252D:?
V3388  SGR    P=125D:?/160D:?
V3395  SGR    P=159D:?
V3412  SGR    CM./SEE V2830 SGR.
V3433  SGR    P=287.0D?
V3443  SGR    P=177.6D?
V3444  SGR    P=160D:?
V3459  SGR    P VAR. CM./SEE V818 SGR.
V3467  SGR    CM./SEE V2947 SGR.
V3473  SGR    SR?
V3500  SGR    CM./SEE V2947 SGR.
V3501  SGR    MIN II 15.7:.
V3508  SGR    EH PACCEHHOO CKOEH/THE MEMBER OF THE
              OPEN CLUSTER M25 (IC 4725).
V3511  SGR    CM./SEE V2947 SGR.
V3536  SGR    P=239.5D?
V3537  SGR    P=318.0D?
V3551  SGR    P=165.2D?/201.0D?
V3560  SGR    P=181D:?
V3564  SGR    CM./SEE V2830 SGR.
V3566  SGR    P=249.0D?
V3583  SGR    P=228.0D?
V3588  SGR     CA/H!=-0.69.
V3625  SGR    P=294D:?
V3634  SGR    P=145D:?
V3645  SGR    CM./SEE Y SGR.
V3709  SGR    P=240.0D?
V3718  SGR    P VAR. EMEHT COEPAT KBAPATH EH:/THE-
              RE IS A NONLINEAR TERM IN THE ELEMENTS:
              +0.865D*10**-10*E**2.
V3748  SGR    P=0.305327D?
V3765  SGR     CA/H!=-0.78.
V3783  SGR    CM./SEE V2028 SGR.
V3784  SGR    P=176.4D?
V3788  SGR    CM./SEE CC SGR.
              KPACHA./RED.
V3791  SGR    CM./SEE AU SGR.
V3792  SGR    VB A (B 8.92M, 13.3", 90G). MIN II 6.81. AH PEE-
               MEHEH CMMAPHOO ECKA./THE RANGE OF
              THE COMBINED LIGHT VARIATION IS GIVEN IN THE TABLE.
              CM./SEE V818 SGR.
V3804  SGR    OCAHE CEKTPA/SPECTRUM DESCRIPTION  6495, 7099!.
V3811  SGR    P2=4D? OCAHE CEKTPA/SPECTRUM DESCRIPTION
               7099, 9845!.
V3817  SGR    VB A (B 16M).
V3819  SGR    P VAR. EMEHT COEPAT KBAPATH EH:/
              THERE IS A NONLINEAR TERM IN THE ELEMENTS:
              +10**-10*E**2.
V3829  SGR    K CTHK./A CLOSE COMPANION.
V3832  SGR    CM./SEE V3829 SGR.
V3834  SGR    EEA  ATMEHHA?/CEPHEID OR ECLIPSING?
V3837  SGR    P=0.565D?  6383!.
V3838  SGR    VB A (B 15.8M).
V3841  SGR    P VAR. MAX=2431970+358D*E (J.D.2423900-33000);
              OCE/SINCE J.D.2433000-CM.TA./SEE TABLE.
V3842  SGR    BOMOHO HAE KOO CTHKA CEKTPAHOO
              KACCA M2?/A CLOSE COMPANION WITH M2? SPECTRAL
              CLASS POSSIBLY EXISTS.
V3843  SGR    CM./SEE V2358 SGR.
V3853  SGR    V22 (NGC 6656=M22). EH TOO APOBOO CKOE-
              H./THE MEMBER OF THIS GLOBULAR CLUSTER.
V3855  SGR    V31 (NGC 6655=M22). BOMOH EH CKOEH./
              POSSIBLE MEMBER OF THE CLUSTER.
V3857  SGR    COACHO  6278!, CEKTP-M8./ACCORDING TO  6278!
              THE SPECTRAL CLASS IS M8.
V3867  SGR    O KAPTO OOHO KAAHO S4903 BMECTO
              CSV 4309./UNDER THE CHART S 4903 IS PRINTED ERRONEO-
              USLY INSTEAD OF CSV 4309.
V3868  SGR    P VAR. MAX=2426130+270D*E (J.D.2423900-33900);
              OCE/SINCE J.D.2435700-CM.TA./SEE TABLE.
V3874  SGR    P VAR. MAX=2436035+115.3D*E (J.D.2426000-38000);
              OCE/SINCE J.D.2438000-CM.TA./SEE TABLE.
V3875  SGR    P VAR. P=358D (J.D.2424000-33800); OCE/SINCE
              J.D.2435000-CM.TA./SEE TABLE.
V3876  SGR    P VAR. MAX=2430090+345D*E (J.D.2423900-32000);
              MAX=2436830+358D*E (J.D.2436000-41500)  6279!;
              OCE/SINCE J.D.2441400-CM.TA./SEE TABLE.
V3879  SGR    VB (DM=2.6M, RO=0.6").
V3880  SGR    OH, SIO, H2O MAEP/MASER.
V3885  SGR    PORB=0.206D  4939!.
              KPOME HEPABHO EPEMEHHOCT, HOA HA-
              ATC BCOKOACTOTHE KOEAH C P1=29.0S,
              P2=30.15S  AMTAM 0.00028M. B CEKTPE-
              OEH POKE H OOEH HI  HEI  MC-
              COHHE KOMOHEHT  AMEPOBCKX H. X-C-
              TOHK./BESIDES THE IRREGULAR VARIABILITY HIGH-FRE-
              QUENCY OSCILLATIONS ARE SOMETIMES OBSERVED WITH
              P1=29.0S, P2=30.15S AND WITH AMPLITUDES OF 0.00028M.
              IN THE SPECTRUM THERE ARE EXTREMELY BROAD ABSORPTION
              LINES OF HI AND HEI. THE BALMER LINES HAVE EMISSION
              COMPONENTS. X-RAY SOURCE.
V3886  SGR    T/TYPE EB?
V3893  SGR    CBAHA C KOEBO TMAHHOCT./CONNECTED WITH
              A RING NEBULA.
V3894  SGR    MIN II 6.37. P VAR?
V3899  SGR    CM./SEE AU SGR.
V3900  SGR    V7 (NGC 6522). HE EH TOO APOBOO CKOEH.
              /NOT A MEMBER OF THIS GLOBULAR CLUSTER.
V3903  SGR    EH PACCEHHOO CKOEH/THE MEMBER OF THE
              OPEN CLUSTER COLLINDER 367.
              B TMAHHOCT/IN THE NEBULA SIMEIS 188.
V3907  SGR    CM./SEE V1389 SGR.
V3929  SGR    P.K.5-5G2.
V3961  SGR    SB1 (PORB=690D  9915!).
V4024  SGR    SB.
V4032  SGR    HEAEKO OT V1309 SGR./NOT FAR FROM V1309 SGR.
V4034  SGR    CM./SEE V1845 SGR.
V4046  SGR    BCK/FLARES (11.1M-12.4M U).
V4048  SGR    MIN II 12.6; DII=0.15P.
V4051- V4056  SGR B PAOHE APOBOO CKOEH/IN THE REGION
              OF THE GLOBULAR CLUSTER NGC 6638.
              HE EH CKOEH./NOT A MEMBER OF THE
              CLUSTER.
V4058  SGR    D=0.02P
V4060  SGR    P VAR. MAX=2437846+283D*E (J.D.2436030-38970);
              OCE/SINCE J.D.2438970-CM.TA./SEE TABLE.
V4066  SGR    D=0.07P.
V4067  SGR    V32 (NGC 6656=M22). HE EH APOBOO CKOEH.
              /NOT A MEMBER OF THE GLOBULAR CLUSTER.
V4068  SGR    V17 (NGC 6656=M22). HE EH APOBOO CKOE-
              H./NOT A MEMBER OF THE GLOBULAR CLUSTER.
V4069  SGR    V33 (NGC 6656=M22). HE EH APOBOO CKOEH.
              /NOT A MEMBER OF THE GLOBULAR CLUSTER.
ETA    SGR    VB A (B 8.0M, 3.5",105G); MU ALFA=-0.0107S,MU             .
DELTA=-0.166"
MU     SGR    VB A (B 10.48M, 16.9", 285G; C 13.0M, 25.2", 119G;
              D 9.69M, 48.5", 312G; E 9.25M, 50.0", 115G). SB 2
              (E=0.4).
              T EPEMEHHOCT/THE VARIABILITY TYPE IS EA/GS+
              +ACYG.
              COACHO  9922!, HAATC TAKE KBAEPO-
              ECKE MEHEH ECKA C AMTO 0.08M-
              0.15M  KAM OT 16D O 40D./ACCORDING TO  9922!
              THERE ARE ALSO QUASIPERIODICAL LIGHT VARIATIONS WITH
              THE AMPLITUDES 0.08M-0.15M AND CYCLES FROM 16D TO
              40D.
IPSILO SGR    MIN II 4.59.
R      SCO    V7 (NGC 6093=M80). BEPOTHA BEA O./PRO-
              BABLE FIELD STAR.
              P VAR. MAX=2400518+220.2D*E (J.D.2400500-04000)
               0960!; MAX=2404493+225.86D*E (J.D.2404000-
              08600); MAX=2409003+222.29D*E (J.D.2408600-
              33300); OCE/SINCE J.D.2433300-CM.TA./SEE
              TABLE.
S      SCO    V6 (NGC 6093=M80). HE EH CKOEH./CLUSTER
              NON-MEMBER.
              P VAR. MAX=2400986+177.00D*E (J.D.2400900-17500);
              OCE/SINCE J.D.2417500-CM.TA./SEE TABLE.
T      SCO    4.0" N, 2.7" E OT EHTPA APOBOO CKOEH
              NGC 6093=M80./4.0" N, 2.7" E FROM THE CENTER OF THE
              GLOBULAR CLUSTER NGC 6093=M80.
U      SCO    PEE BCK/PREVIOUS OUTBURSTS:
              2401646: (1863), 2417343 (1906), 2428342 (1936).
Y      SCO    C 1972 . MEHETC ECK B PEEAX 12.3M-15.0M HE-
              PEPHO, MAKCMM HEPECKAEM/SINCE 1972
              VARIES ITS BRIGHTNESS IN THE RANGE 12.3M-15.0M IRREGU-
              LARLY, MAXIMA ARE UNPREDICTABLE  8080!.
Z      SCO    P VAR. MAX=2425546+357.17D*E (J.D.2412500-
              25600); OCE/SINCE J.D.2430000-CM.TA./SEE
              TABLE.
RR     SCO    SIO MAEP/MASER.
              P VAR. MAX=2416944+284.31D*E (J.D.2411000-
              18000); MAX=2422828+278.09D*E (J.D.2422800-
              40000); OCE/SINCE J.D.2440000-CM.TA./SEE
              TABLE.
RU     SCO    P VAR. B HTEPBAE/DURING J.D.2425000-40000-CM.
              TA./SEE TABLE.
RV     SCO    VB A (B 13.0M, 5.9", 325G).
RW     SCO    OH, H2O, SIO MAEP/MASER.
RY     SCO    P VAR, KBAPATH EH/NONLINEAR TERM:
              +4.10D*10**-6*E**2.  A/H!=0.2.
              VB A (B 10.70M, F8:, 13.8", 220.5G, 1965;
              C 11.5M, 2.0", 102G, 1964; D 11.43M, 24", 80G). AH
              CMMAPH ECK AC./COMBINED BRIGHTNESS OF AC IS
              GIVEN.
RZ     SCO    P VAR. MAX=2413994+161.20D*E (J.D.2413600-
              22700); MAX=2422858+155.79D*E (J.D.2422700-
              28000); MAX=2428156+160.29D*E (J.D.2428000-
              35000); OCE/SINCE J.D.2437500-CM.TA./SEE
              TABLE.
SV     SCO    P VAR. MAX=2418886+258.5D:*E (J.D.2411600-
              19000); MAX=2424233+252.43D*E (J.D.2420500-
              28600); MAX=2429055+255.9D:*E (J.D.2428600-
              35000); OCE/SINCE J.D.2437000-CM.TA./SEE
              TABLE.
SY     SCO    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6475=M7.
TX     SCO    CM./SEE SY SCO. BEPOTH EH CKOEH./PRO-
              BABLE CLUSTER MEMBER.
XX     SCO    EMEHTAM/THE ELEMENTS MAX=2413786+152D*E
               0031! HAEH  9447! HE PECTABTC./DO
              NOT REPRESENT THE OBSERVATIONS FROM  9447!.
AC     SCO    COACHO/ACCORDING TO  0266!, CST:, 12.2M-12.6M PG.
AH     SCO    OH, H2O, SIO MAEP/MASER.
AI     SCO    P2=966.6D.
AL     SCO    MIN II 11.3.
AN     SCO    BOMOEH T EA./EA TYPE IS POSSIBLE.
AP     SCO    COACHO/ACCORDING TO  9447!, 13.5M-14.2M PG;
              EHTKA COMHTEHA./DOUBTFUL IDENTIFICATION.
AR     SCO    COACHO  7104!, CEKTP TA T TAU./ACCORDING TO
               7104!, T TAU TYPE SPECTRUM.
AU     SCO    VB A (B=V725 SCO, 0.4', 0G).
AV     SCO    KAPTA  CBEEH B  9447! OTHOCTC K PO
              BEE./THE CHART AND DATA IN  9447! CORRESPOND TO
              ANOTHER STAR.
BI     SCO    VB B (A=GW SCO; B 6", 150G).
BM     SCO    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6405=M6.
BN     SCO    CM./SEE SY SCO.
              OXOA HA R CEN./RESEMBLES R CEN.
BS     SCO    D<=0.03P. COACHO/ACCORDING TO  0021!, SP F8.
BT     SCO    P VAR. PBEEHHE B TAE EMEHT COEPAT
              CHCOAH EH:/THERE IS PERIODIC TERM IN
              THE ELEMENTS GIVEN IN THE TABLE:+0.05D SIN (176G+
              +0.0857G*E).
              EKT AKO?/BLAZHKO EFFECT?
BV     SCO    EHTKA B  9447! COMHTEHA./DOUBTFUL
              IDENTIFICATION IN  9447!.
CF     SCO    MIN II 13.8.
CK     SCO    VB A (B 15M, 14").
CL     SCO    ECK B OTECKOM   AAOHE MOPOBAH
              C EMEHTAM/THE BRIGHTNESS IN OPTICAL AND UV RAN-
              GE IS MODULATED ACCORDING TO THE ELEMENTS: MIN (PG)=
              =2427020+624.7D*E.
              BCK/OUTBURSTS 1892, 1899, 1907, 1926.
CP     SCO    N=4.
CQ     SCO     A/H!=-1.4.
DX     SCO    VB A (B P).
EZ     SCO    VB A (B 15.6M NF).
FQ     SCO    VB A (B 16M VIS).
FU     SCO    VB A (B NP).
              MIN II 12.7, MIN II-MIN I=0.493P.
FV     SCO    D=0.015P. HA MIN II/DEPTH OF MIN II 0.1M PG.
FY     SCO    VB A (B 15M, 15", 35G).
GG     SCO    VB A (B 15M, 8", 45G).
GM     SCO    CEBEPHA  BX BE, OTMEEHHX HA KAPTE 
              C 1677./THE NOTHERN ONE OF THE TWO STARS NOTED
              ON THE CHART FOR C 1677.
GW     SCO    VB A (B=BI SCO, 6", 150G).
IU     SCO    VB A (B 16.4M NF).
              MAX=2413280+69.05D*E (1893-1906);
              B HTEPBAE/DURING 1910-1928-CM.TA./SEE
              TABLE.
KO     SCO    CTPE MEHEH/RAPID VARIATIONS: A=1.0M.
              MEEHHE KOEAH/SLOW CHANGES:
              A=0.5M, P=2000D+-.
KQ     SCO     A/H!=+0.3. P VAR?
LO     SCO    P VAR? O/BEFORE J.D.2419150 MAX=2411500+450D*E;
              OCE/SINCE J.D.2423900-CM.TA./SEE TABLE.
              CEKTP OE M5./THE SPECTRUM IS LATER THAN M5.
LR     SCO    CEKTP OOEH RCRB B MAX ECKA  8090!. K -
              TOK. MHMM TA RCB HE HAAC./THE
              SPECTRUM RESEMBLES RCRB IN MAX LIGHT  8090!.
              IR EXCESS. RCB TYPE MINIMA WERE NOT OBSERVED.
OO     SCO    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER TR 29.
QZ     SCO    P VAR. O/BEFORE J.D.2420400 MAX=2412640+158D*E;
              OCE/SINCE J.D.2423900-CM.TA./SEE TABLE.
V347   SCO    P VAR. O/BEFORE J.D.2418700 MAX=2411500+198D*E;
              OCE/SINCE J.D.2423900-CM.TA./SEE TABLE.
V381   SCO    D=0.046P.
V382   SCO    CM./SEE SY SCO.
V385   SCO    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER CR 338.
V387   SCO    MIN II 12.2.
V390   SCO    P VAR. O/BEFORE J.D.2422500 MAX=2420330+466D*E;
              OCE/SINCE J.D.2423900-CM.TA./SEE TABLE.
V393   SCO    MIN II 8.3.
V400   SCO    MIN II 15.0.
V402   SCO    CM./SEE SY SCO.
V403   SCO    D=0.02P. HA MIN II/THE DEPTH OF MIN II 0.05M.
V407   SCO    CM./SEE SY SCO.
V411   SCO    MIN II 14.0.
V412   SCO    MIN II 14.8. CM./SEE SY SCO.
V420   SCO    CM./SEE SY SCO.
V421   SCO    P VAR. O/BEFORE J.D.2418000 MAX=2413830+293D*E;
              OCE/SINCE J.D.2423900-CM.TA./SEE TABLE.
V423   SCO    MIN II 14.2. CM./SEE SY SCO.
V425_  V426   SCO CM./SEE SY SCO.
V429   SCO    CM./SEE SY SCO.
V430   SCO    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER TR 30.
V432   SCO    CM./SEE V430 SCO.
V437   SCO    D=0.02P. MIN II 13.9.
V438   SCO    OOEH EPEMEHHO HA KAPTAX  0021!   6286!
              PACXOTC./POSITIONS OF THE VARIABLE IN THE CHARTS
               0021! AND  6286! DIFFER.
V439   SCO    P VAR. O/BEFORE J.D.2418200 MAX=2413350+166.5D*E;
              OCE/SINCE J.D.2419900-CM.TA./SEE TABLE.
V440   SCO    CM./SEE V430 SCO.
V446   SCO    P VAR? O/BEFORE J.D.2435000 MAX=2434980.1+
              +28.6195D.  A/H!=-1.0.
V450   SCO    A=0.9M PG.
V453   SCO    VB A (B 13.51M, F7V, 13.5", 168G). MIN II 6.70.
              OPMA KPBO ECKA/THE LIGHT CURVE SHAPE VAR?
V455   SCO    P.K.351G+3G1. PHAEHOCT K AHETAPHM T-
              MAHHOCTM COMHTEHA. HOBOOOHE BCK C
              HTEPBAOM B HECKOKO ET./PLANETARY NEBULA NATU-
              RE IS DOUBTFUL. NOVA-LIKE OUTBURSTS SEPARATED BY SE-
              VERAL YEARS.
V457   SCO    MIN II 11.3.
V460   SCO    D=0.02P.
V464   SCO    D=0.03P.
V466   SCO    MIN II 13.7.
V467   SCO    P VAR. P=2.41354D (1889-1903); OCE/SINCE 1903-
              CM.TA./SEE TABLE.
V470   SCO     A/H!=0.1.
V471   SCO    MIN II 15.2, DII=0.08P( ).
V472   SCO    D=0.02P.
V474   SCO    MIN II 10.6.
V483   SCO    CI=+3.5M.
V485   SCO    HAKABATC OEE CTPE KOEAH./SHORT
              TERM VARIATIONS ARE SUPERIMPOSED.
V486   SCO    D>=4D? P=1D BOMOEH/IS POSSIBLE.
              B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6383.
V487   SCO     FE/H!=-1.67, DS=9.0.
V490   SCO    MIN II 12.5.
V491   SCO    MIN II 13.2.
V494   SCO    A VAR (1.27M-1.66M B). P VAR? DS=2.
              VB A (B 12.72M Y, 23").
V495   SCO    CM./SEE V485 SCO (DMSHORT=0.5M+-).
V496   SCO    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6414.
              D=0.03P.
V497   SCO    MIN II 13.6.
V499   SCO    AII=0.47M V. MIN I-MIN II=0.504P.
V502   SCO    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER C 1712-407.
V507   SCO    OXA MAX   0300! HE COACETC C EMEHTAM./
              THE EPOCH OF MAX FROM  0300! CONTRADICTS THE ELE-
              MENTS.
V540   SCO    VB A (B 15.2M SP).
V547   SCO    VB B (A 14.2M SF).
V549   SCO     A/H!=-1.1.
V555   SCO     A/H!=-0.3.
V562   SCO    MIN II 12.1.
V566   SCO    D=0.01P:.
V567   SCO    VB A (B 13.01M, 10"SP, CD 30"NF). P VAR.
V568   SCO    D=0.04P.
V569   SCO    MIN II 11.4.
V570   SCO    P VAR?
              HEOHO POK MAX./UNUSUALLY BROAD MAX.
V573   SCO    D=0.06P. CM./SEE V574 SCO.
V574   SCO    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER TR 24.
V575   SCO    MIN II 12.4.
V579   SCO    CM./SEE V574 SCO.
V581   SCO    MIN II 11.9.
V584   SCO    MIN II 13.1.
V585   SCO    D=0.03P:.
V586   SCO    D=0.04P. CM./SEE V574 SCO.
V588   SCO    D=0.02P. CM./SEE V574 SCO.
V589   SCO    D=0.05P. CM./SEE V574 SCO.
V590   SCO    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6231.
V592   SCO    MIN II 13.3.
V593   SCO    D=0.05P:.
V594   SCO    D=0.01P.
V603   SCO    D=0.04P.
V606   SCO    D=0.07P.
V607   SCO    MIN II 10.3.
V609   SCO    MIN II 13.7.
V611   SCO    D=0.04P. MIN II 13.7.
V612   SCO    D=0.05P.
V613   SCO    D=0.04P.
V616   SCO    MIN II 12.4.
V619   SCO    MIN II 12.1.
V620   SCO    D=0.02P.
V621   SCO    D=0.04P.
V622   SCO    MIN II 14.2.
V623   SCO    TEHOE BPEM E MEHEH B MAX, HOA
              EAETC CAO./LONG INTERVALS IN MAX WITHOUT
              CHANGES, SOMETIMES BECOMES FAINT.
V625   SCO    VB A (B 13.2M SF). MIN II 13.5.
V627   SCO    MIN II 14.1.
V628   SCO    MIN II 12.4.
V629   SCO    BEHE H AC./APSIDAL MOTION.
V631   SCO    MIN II 13.2.
V632   SCO    D=0.06P.
V633   SCO    MIN II 12.2.
V634   SCO    MIN II 12.2.
V636   SCO    SB1 (PORB=1318D).
V638   SCO    D=0.07P.
V640   SCO    MIN II 13.5.
V660   SCO    VB A (B 16.0M S).
V672   SCO    P=180D BOMOEH/IS POSSIBLE.
V674   SCO    VB A (B 15.0M S).
V679   SCO    P=364D BOMOEH/IS POSSIBLE.
V690   SCO    VB A (B 14.40M Y, 6", 0G). AH PEE CMMAPHO-
              O ECKA./THE RANGE OF THE COMBINED LIGHT IS GIVEN.
              DS=4.
V698   SCO    D<=0.20D, D=0.043D.
V700   SCO    MIN II 10.3.
V701   SCO    MIN II 9.05. P VAR. MIN I=2439329.6657+0.76187133D*E
              (J.D.2428000-39400)  7177!; OCE/SINCE
              J.D.2439400-CM.TA./SEE TABLE.
              CM./SEE V702 SCO.
V702   SCO    BEPOTH EH PACCEHHOO CKOEH/PROBABLE
              MEMBER OF THE OPEN CLUSTER NGC 6383.
V703   SCO    P0=0.1499615D  3521!; P1-CM.TA./SEE TABLE
              (P VAR?). OTMEAC TAKE/ALSO NOTED P=
              =0.04162025D  3521!. A VAR (0.23M-0.46M).
              EH/BEAT PHENOMENON: MAX=2436760.249+
              +0.497306D*E  3521!. DS=1.
              CM./SEE BM SCO.
V705   SCO    MIN II 14.1:.
V706   SCO    MOMEHT MAX   0046! HE COACTC C TA-
              HM EMEHTAM. B  4678! HAEHO A<=0.05M V A
              6 HOE./MOMENTS OF MAX FROM  0046! CONTRADICT THE
              TABULATED ELEMENTS. ACCORDING TO  4678!, A<=0.05M V
              DURING 6 NIGHTS.
V708   SCO    CM./SEE SY SCO.
V709   SCO    CM./SEE SY SCO.  A/H!=-0.6.
V710   SCO    MIN II 14.2.
V711   SCO    CM./SEE SY SCO.
V712   SCO    MIN II 14.0.
V714   SCO    D=0.05P:. CM./SEE V732 SCO.
V717   SCO     A/H!=0.9.
V718   SCO    D=4D. EE OH/ANOTHER MIN 2429847-849  0270!.
V720   SCO    CM./SEE SY SCO.
V723   SCO    CM./SEE SY SCO. HA KPA TEMHOO OAKA./AT THE
              EDGE OF A DARK CLOUD.
V725   SCO    VB B (A=AU SCO, B 0.4', 0G).
V729   SCO    BOMOHO, HOBA./POSSIBLY A NOVA.
V732   SCO    P MOET T BBOE OE./P MAY BE TWICE LONGER.
V733_  V734   SCO CM./SEE V729 SCO.
V735   SCO    OPMA KPBO ECKA MEHETC/THE LIGHT CURVE
              SHAPE VAR.
V738   SCO    D=0.04P:; MIN II 13.4:. CM./SEE SY SCO.
V740   SCO    CM./SEE SY SCO.
V749   SCO    P=410D BOMOEH/IS POSSIBLE.
V756   SCO    MIN II 10.7.
V760   SCP    DI=0.02P; MIN II 7.4; DII=0.2P:, DII=0.03P.
V761   SCO    HE CKEH T IN./IN TYPE IS NOT EXCLUDED.
V764   SCO    MIN II 9.0.
V805   SCO    BOMOHO, P BBOE KOPOE./POSSIBLY P IS TWICE
              SHORTER.
V818   SCO    SCO X-1. SB.
              VAR PEHTEHOBCK  MHOOKOMOHEHTH PAOC-
              TOHK./VAR X-RAY AND MULTI-COMPONENT RADIO SOUR-
              CE. LX/LBOL=300-1000.
              AHA OXA MIN EPOECKO COCTABE EC-
              KA (A=0.25M). KTA ECKA  BCK O 1M
              A BPEM ECTK CEKH-MHT. B CEPEHE
              1960-X OOB CPEH POBEH ECKA OHC HA
              0.3M-0.4M. B CEKTPE-OO KOHTHM  MC-
              C H, HEI, HEII, CIII, NIII./THE EPOCH OF MIN IS
              GIVEN FOR THE PERIODIC COMPONENT OF THE LIGHT VARIATI-
              ON (A=0.25M). FLICKERING AND FLARES UP TO 1M WITH
              TIME SCALE FROM DOZENS OF SECONDS TO MINUTES. THE
              MEAN BRIGHTNESS LEVEL DECREASED IN THE MIDDLE OF
              1960-ES BY 0.3M-0.4M. THE SPECTRUM WITH BLUE CONTI-
              NUUM AND H, HEI, HEII, CIII, NIII EMISSIONS.
V819   SCO    MIN II 13.2.
V821   SCO    MIN II 14.5.
V822   SCO    VB? CMMAPH ECK./COMBINED BRIGHTNESS.
V827   SCO    MIN II 14.1.
V833   SCO    MIN II 11.2.
V837   SCO    D=0.03P:; MIN II 14.3.
V838   SCO    MIN II 13.4.
V842   SCO    MIN II 12.3.
V843   SCO    MIN II 10.5.
V848   SCO    MIN II 13.1. BOMOEH T RRC C OOBHHM EP-
              OOM./RRC TYPE WITH TWICE SHORTER PERIOD IS POSSIB-
              LE.
V849   SCO    MIN II 14.1.
V853   SCO    D=0.05P; MIN II 14.1.
V856   SCO    VB C (A=BS 6000, 6.65M, AO-3III; B 12.55M, 16",
              298G; C 44", 185G; D 11.7M, CD 1.3", 105G, 1945).
V857   SCO    OOHO OOHAEHA "10" (BMECTO "11") HA KAPTE.
              /ERRONEOUSLY LABELLED "10" (INSTEAD OF "11") IN THE
              CHART.
V858   SCO    OOHO OOHAEHA "11" (BMECTO "10") HA KAPTE.
              /ERRONEOUSLY LABELLED "11" (INSTEAD OF "10") IN THE
              CHART.
V861   SCO    SB1. MIN II 6.28. H MHMMOB MEHTC./
              DEPTHS OF MINIMA VAR.
              B OACT PACCEHHX CKOEH/IN THE REGION OF
              OPEN CLUSTER NGC 6231, CR 316, TR 24.
V862   SCO    OHO/USUALLY 6.67M-6.76M.
              BCKA POOTEHOCT 40M 3  1965./
              A FLARE OF 40M DURATION ON JULY 3, 1965.
              CM./SEE BM SCO.
V866   SCO    VB (DM-0.5M, -1", 200G). M (6370 A)=11.14M-12.37M.
              K TOK./IR EXCESS.
V870   SCO    B-V=+3.38M-+3.52M. CM./SEE V590 SCO.
V877   SCO    MIN II 13.1.
V883   SCO    VB A (B 12.60M, 9", 130G). P VAR?
              MIN=2438228.315+1.294745D*E (J.D.2438200-40500)
               6871!; OCE/SINCE J.D.2440500-CM.TA./SEE
              TABLE.
              OK/DEEP MIN II.
V884   SCO    4U 1700-37. LX/LBOL=0.00007. ATMEHH X-C-
              TOHK. POOTEHOCT ATMEH VAR:
              0.61D<=DX<=1.10D. AH MOMEHT CEPEH PEHTEHOBC-
              KOO ATMEH, COBAA C MIN II. PEHTEHOBC-
              K OTOK VAR B KAE OT CEKH O ACOB. BPEME-
              HAM POCEBAETC MO C P=97 MH, AM-
              TA KOTOPO B OTKE OCTAET DV=0.01M./
              ECLIPSING X-RAY SOURCE. ECLIPSE DURATION IS VARIABLE
              IN THE RANGES 0.61D<=DX<=1.10D. THE EPOCH OF THE MIDD-
              LE OF THE X-RAY ECLIPSE COINCIDING WITH MIN II IS GI-
              VEN. X-RAY FLUX VAR IN THE SCALE FROM SECONDS TILL
              HOURS. SOMETIMES A PERIODIC MODULATION WITH P=97
              MIN IS PRESENT, ITS AMPLITUDE IN THE OPTICAL BAND REA-
              CHES DV=0.01M.
              MIN II 6.57; MIN I-MIN II=0.63P, DI=0.2P.
              OKPEHA KOEBO TMAHHOCT SH 2. B PAOHE
              PACCEHHOO CKOEH NGC 6281. BEA O./
              SURROUNDED BY THE RING NEBULA SH 2. IN THE REGION OF
              THE OPEN CLUSTER NGC 6281. FIELD STAR.
V885   SCO    AMETH/NOTICEABLE MIN II.
V889   SCO    CEBEPH KOMOHEHT TPOHO./THE NORTHERN COMPO-
              NENT OF A TRIPLE.
V890   SCO    VB A (B 11.5M, 0.5' N).
V894   SCO    A=0.6M PG.
V896   SCO    BOMOHO, HEBEPH KOOPHAT  KAPTA./CO-ORDI-
              NATES OR THE CHART MAY BE ERRONEOUS.
V900   SCO    CM./SEE V590 SCO.
              KPBA ECKA-CHCOAHA BOHA. BOMOH
              EPO/THE LIGHT CURVE IS A SINUSOIDAL WAVE. POSSIB-
              LY P=6.20D; 6.85D.
V903   SCO    N96  2448!. HEBEPHO OTOECTBEHA C/ERRONEOUSLY
              IDENTIFIED WITH V479 SCO.
V906   SCO    CM./SEE SY SCO. BEPOTH EH CKOEH./PROBAB-
              LE CLUSTER MEMBER. VB (DMV=0.8M, 0.1", 111G, 1957).
              AH PEE MEHEH CMMAPHOO ECKA./THE
              RANGE OF THE COMBINED LIGHT VARIATION IS GIVEN.
              MIN II 6.21.
V907   SCO    CM./SEE SY SCO. MIN II 9.2.
V911   SCO    PO BOMOH P/ALTERNATIVE P=4.2D.
V913   SCO    PO BOMOH P/ALTERNATIVE P=0.976D.
              K TOK/IR EXCESS.
V914   SCO    VB (DMV=2M, 3", 200G).
              CHCOAHA BOHA C P/SINE WAVE WITH P=2.69D,
              DB=0.15M (B=12.91M)  9753!.
V915   SCO    VB A (B 10.43M, WN6, 14", 330G; C 11.40M, 20", 202G;
              D 13.96M, 22", 80G, 1973). ECK MEHC OT
              6.32M O 6.50M A BPEM C J.D.2443680 O 44115./
              THE BRIGHTNESS DECREASED FROM 6.32M TO 6.50M DURING
              J.D.2443680-44115.
V917   SCO    VB A (B 17M: SP). BCKA: O'EM ECKA 1930-
              1936, MAX 1936-1938, CA 1938-1952./THE OUT-
              BURST: RISE 1930-1936, MAX 1936-1938, DECLINE
              1938-1952.
V919   SCO    CM./SEE V590 SCO.
V920   SCO    CM./SEE V590 SCO.
              MHOECTBEHHA EPOHOCT:/MULTIPLE PERIODICI-
              TY: P1-CM.TA./SEE TABLE, OAMTA/SEMI-
              AMPLITUDE A1=0.0051M; P2=0.10765D. A2=0.0046M;
              P3=0.10388D, A3=0.00485M; P4=0.12137D, A4=
              =0.0036M; P5=0.6929D?, A5=0.0028M.
V921   SCO    BEA OCBEAET TMAHHOCT./THE STAR ILLUMINATES
              A NEBULA.
V922   SCO    MHOECTBEHHA EPOHOCT, HAKABATC A-
              CTOT C AMTAM 0.0010M-0.0352M./MULTIPLE PE-
              RIODICITY, SUPERPOSITION OF FREQUENCIES WITH AMPLITUDES
              0.0010M-0.0352M.
V923   SCO    D=0.32D:. EMEHT HATC B OTBEPEH./
              THE ELEMENTS NEED CONFIRMATION.
              B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6281.
V924   SCO    B-V VAR:+1.90, +2.50,
              KTA ECKA HA 0.1M-0.2M (U, B) B TEEHE M-
              HT./LIGHT FLUCTUATIONS BY 0.1M-0.2M (U, B) IN SEVERAL
              MINUTES.
V925   SCO    VB A (B-10", CA, OO/FAINT, BLUE). BEPOT-
              H EH PACCEHHOO CKOEH/PROBABLE MEMBER
              OF THE OPEN CLUSTER TR 27.
              O VR BOMOHE HAEH P/IN VR POSSIBLE VALUES
              OF P: 105.3D, 73.0D, 188.7D, 312.5D  9950!.
V926   SCO    3U 1735-44=SCO XR-3. BCK HAKABATC
              HA HEOE MEHEH ECKA C P=0.18D, B-
              MC, O-BMOM, OPTAHM  4394!./BURSTS
              SUPERIMPOSE SMALL LIGHT VARIATIONS WITH P=0.18D
              WHICH IS APPARENTLY THE ORBITAL PERIOD  4394!.
V927   SCO    AHA OXA MIN B AX U. K TOK./THE EPOCH
              OF MIN IN U LIGHT IS GIVEN. IR EXCESS.
ALFA   SCO    ADS 10074 A(B 5.1M, B4VE, A=2.9", PORB=878 YR.).
              CBAHA C TMAHHOCT./CONNECTED WITH A NEBULA.
DZETA* *1     SCO CM./SEE V590 SCO.
KAPPA  SCO    SB. P2=0.205430D. P1 VAR. EH/BEAT PHENOMENON:
              =7.3316D.
LAMBDA SCO    SB 1. PORB=5.6D? APULS=0.02M. OOEPOECKE
              MEHEH ECKA:/LONG PERIOD LIGHT CHANGES:
              MAX=2440376.15+10.1605D*E  9761!. OHAPEHO
              OHO ATMEHE/ONE ECLIPSE WAS FOUND (J.D.2440690,
              A-0.04M)  6388!.
MU**1  SCO    MIN II 3.12.
SIGMA  SCO    VB AA (A 5.5M, 0.37", 96G, 1981, OPTAHOE BE-
              HE?/ORBITAL MOTION?; B 8.45M, B9.5V, 20.1", 273G,
              1961); SB1, PORB=33.06D. P0 VAR.
              MAX VR=2420000.1465+0.24682815D*E (1918-1924)
               9953!; MAX=2432306.918+0.246846D*E (J.D.
              2432000-37800)  9764!; OCE/SINCE J.D.2437800-
              CM.TA./SEE TABLE.
              A0=0.036M Y. P1=0.2396674D, A1=0.013M Y  9762!.
              PBEAT=8.256D=PORB/4  9957!.
              CBAHA C TMAHHOCT./CONNECTED WITH A NEBULA.
R      SCL    VB A (B 19.9M, 10", 234G). CO MCC/EMISSION.
S      SCL    P VAR. MAX=2412774+367.9D*E (J.D.2405400-20500);
              MAX=2423035+360.6D*E (J.D.2421250-27740);
              MAX=2427738+370.4D*E (J.D.2427700-34000)  0960!;
              OCE/SINCE J.D.2434000-CM.TA./SEE TABLE.
              H2O MCC/EMISSION.
T      SCL    P VAR. MAX=2417400+202.26D*E (J.D.2411300-
              19000); MAX=2420390+197.85D*E (J.D.2419000-
              23600); OCE/SINCE J.D.2423600-CM.TA./SEE
              TABLE.
V      SCL    P VAR. MAX=2414006+294.8D*E (J.D.2411600-18200);
              MAX=2422866+297.2D*E (J.D.2420400-35100); OCE/
              SINCE J.D.2435100-CM.TA./SEE TABLE.
X      SCL    P VAR. MAX=2413796+258.7D*E (J.D.2413500-22800);
              OCE/SINCE J.D.2422800-CM.TA./SEE TABLE.
Y      SCL    HOA HAATC K 100D:  300D:/
              THE CYCLES 100D: AND 300D: ARE SOMETIMES OBSERVED.
RT     SCL    MIN II 10.47.  FE/H!=-0.75. P VAR. EMEHT, AHHE
              B TAE, COEPAT KBAPATH EH:/THERE IS
              A NONLINEAR TERM IN THE ELEMENTS GIVEN IN THE TABLE:
              -9.04D*10**-11*E**2.
RU     SCL    (K-B)2=0.09. A VAR  3429!. P VAR. MAX=2425094.4175+
              +0.4933257D*E (J.D.2416750-25100)  0183!; MAX=
              =2427403.177+0.4933239D*E (J.D.2425100-30650)
               1381!; OCE/SINCE J.D.2430650-CM.TA./SEE
              TABLE.
RW     SCL    P VAR?
SV     SCL     FE/H!=-1.82. P VAR? MAX=2439468.364+
              +0.3773636D*E (J.D.2427300-39500)  5233!; OCE/
              SINCE J.D.2439850-CM.TA./SEE TABLE.
SY     SCL    H2O MAEP/MASER.
              P VAR? MAX=2426160+411D*E  0193!; OCE/SINCE
              J.D.2440400-CM.TA./SEE TABLE.
SZ     SCL    MIN II 13.68.
UY     SCL    POM C AAKTKO/NEAR THE GALAXY NGC 55.
UZ     SCL    VB A (B 15.81M, 23", 135G); (K-B)2=0.14. CM./SEE
              V818 SGR.
VV     SCL    MIN II 8.50. ACV?  8083!.
VY     SCL    PORB=0.1662D?  9932!. HAATC BCOKE  H-
              KE COCTOH CCTEM./HIGH AND LOW STATES OF THE
              SYSTEM ARE OBSERVED.
VZ     SCL    HAATC BCOKE  HKE COCTOH CCTEM.
              /HIGH AND LOW STATES OF THE SYSTEM ARE OBSERVED
               9933!.
WZ     SCL    HAATC BA KOEAH C EPOAM P1  P2:/
              THERE ARE TWO OSCILLATIONS WITH THE PERIODS P1 AND
              P2: P1=0.06576D, P2=0.095944D, P1/P2=0.6854.
XX     SCL    HAATC BA KOEAH C EPOAM P1  P2:
              /THERE ARE TWO OSCILLATIONS WITH THE PERIODS P1 AND
              P2:P1=0.048898D, P2=0.051350D, P1/P2=0.95225.
AI     SCL    HAATC BA KOEAH C EPOAM P1  P2:/
              THERE ARE TWO OSCILLATIONS WITH THE PERIODS P1 AND
              P2:P1=0.044D, P2=0.0931D, P1/P2=0.47.
AL     SCL    MIN II 6.20; MIN II-MIN I=0.475P; DII=0.08P.
AO     SCL    MU=0.46", P=187G.
R      SCT     FE/H!=-1. P VAR. MIN I=2377165+142.8D*E
              (J.D.2377160-9820); MIN I=2384885+142.6D*E
              (J.D.2384890-8170); MIN I=2394451+141.4D*E
              (J.D.2394450-8500); MIN I=2398777+142.4D*E
              (J.D.2398770-2404320); MIN I=2404627+137.4D*E
              (J.D.2404600-6410); MIN I=2406561+142.7D*E
              (J.D.2406560-9065); MIN I=2409742+143.6D*E
              (J.D.2409730-12700); MIN I=2412755+141.5D*E
              (J.D.2412750-16720); MIN I=2417161+139.5D*E
              (J.D.2417150-20790); MIN I=2421083+143.4D*E
              (J.D.2421050-25170)  9935!; MIN I=2429478+142.8D*E
              (J.D.2429000-30650)  9938!; MIN I=2432078+140.05D*E
              (J.D.2432000-42240)  7596!; MIN I=2442737+152.5D*E
              (J.D.2442550-43050); MIN I=2443315+138.5D*E
              (J.D.2443050-44150)  0001!; OCE/SINCE
              J.D.2444150-CM.TA./SEE TABLE.
              PAK KPBO ECKA/LIGHT CURVE DRAWINGS  9935,
              9936, 9937!.
              OCAHE CEKTPA/SPECTRUM DESCRIPTION  9939, 9954!.
S      SCT    VB A (B 11.9M V, 14.5", 238G; C 12.5M V, 44", 105G).
U      SCT    MIN II 10.31.
W      SCT    MIN II 10.1.
X      SCT     A/H!=-0.1. B PAOHE PACCEHHOO CKOEH/IN THE
              REGION OF THE OPEN CLUSTER NGC 6639.
Y      SCT    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF THE
              OPEN CLUSTER NGC 6664.
Z      SCT     A/H!=0.3.
RS     SCT    MIN II 10.08.
RU     SCT     A/H!=-0.7. P VAR. EMEHT, PBEEHHE B TA-
              E, COEPAT KBAPATH EH:/THERE IS A NONLINE-
              AR TERM IN THE ELEMENTS GIVEN IN THE TABLE:
              +3.15D*10**-6*E**2.
RX     SCT    CBAHA C PKO BOOPOHO TMAHHOCT/CONNEC-
              TED WITH THE BRIGHT HYDROGEN NEBULA YM 13.
RY     SCT    MIN II 9.56. P VAR? MIN I=2427979.340+11.124939D*E
              (J.D.2414800-36100)  0007!; OCE/SINCE
              J.D.2431200-CM.TA./SEE TABLE.
              OPMA KPBO ECKA MEHETC./THE SHAPE OF THE
              LIGHT CURVE VARIES.
RZ     SCT    MIN II 7.47. P VAR. EMEHT, PBEEHHE B TA-
              E, COEPAT KBAPATH EH:/THERE IS NONLINE-
              AR TERM IN THE ELEMENTS GIVEN IN THE TABLE:
              +0.78D*10**-7*E**2.
SU     SCT    P VAR. MAX=2424324.48+1.467713D*E (J.D.2420700-
              34310); MAX=2439678.428+1.468753D*E
              (J.D.2437100-41100)  7806!; OCE/SINCE
              J.D.2441100-CM.TA./SEE TABLE.
TX     SCT    CWA? KPACHA./RED.
TY     SCT     A/H!=-0.3. B PAOHE PACCEHHOO CKOEH/IN THE
              REGION OF THE OPEN CLUSTER TR 35.
UZ     SCT     FE/H!=0.35. P VAR. MAX=2435629.5+14.7468D*E
              (J.D.2423900-35700)  2309!; OCE/SINCE J.D.
              2436000-CM.TA./SEE TABLE.
VV     SCT    SF KOMOHEHT BOHO BE./SF COMPONENT OF A
              PAIR.
VW     SCT    P VAR. MAX=2415887+234D*E (J.D.2411900-22210);
              MAX=2423588+235D*E (J.D.2422880-27600);
              MAX=2429468+235.1D*E (J.D.2428750-34200);
              OCE/SINCE J.D.2434600-CM.TA./SEE TABLE.
VX     SCT    D=0.064P.
VZ     SCT    MIN II 12.0.
WY     SCT    P VAR.
XY     SCT    MIN II 14.5.
AC     SCT    D=0.024P; MIN II 10.2.
AE     SCT    D=0.04P.
AI     SCT    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF THE
              OPEN CLUSTER NGC 6705.
AN     SCT    P VAR?
AP     SCT    V2 (NGC 6712).
AU     SCT    D=0.03P.
BC     SCT    BOCTOH KOMOHEHT TECHO BOHO CCTEM.
              CTHK-NSV 11551./FOLLOWING COMPONENT OF A
              CLOSE DOUBLE SYSTEM. THE COMPANION-NSV 11551.
BH     SCT    MIN II 14.9.
BI     SCT    VB A (B 16.3M:, 3", 280G; C 16.7M:, 12", 190G;
              D 16.8M:, 18", 45G; E 17.0M:, 6", 350G).
BK     SCT    K CTHK/CLOSE COMPANION 16.5M SF.
BN     SCT    D=0.02P.
BP     SCT    S 5.5/5.5.
BS     SCT    MIN II 11.07. B PAOHE PACCEHHOO CKOEH/IN THE
              REGION OF THE OPEN CLUSTER M11 (NGC 6705).
BU     SCT    A VAR. P VAR. MAX=2425804.625+0.42022D*E  1401!;
              MAX=2427928.041+0.4202188D*E (J.D.2427900-
              9440)  1404!; MAX=2432770.464+0.4201944D*E
              (J.D.2432740-38290); MAX=2438589.357+
              +0.4202171D*E (J.D.2438580-40510)  7806!; OCE/
              SINCE J.D.2440770-CM.TA./SEE TABLE.
BX     SCT     A/H!=-0.9.
CD     SCT    MIN II 13.7.
CF     SCT    D=0.035P.
CH     SCT    V7 (NGC 6712). EH TOO APOBOO CKOEH./
              THE MEMBER OF THIS GLOBULAR CLUSTER.
CK     SCT     FE/H!=0.23.
CL     SCT    MOET T, EPO CEET BOT?/MAYBE THE
              PERIOD SHOULD BE DOUBLED?
CM     SCT     A/H!=0.1.
CN     SCT     A/H!=-1.5.
CO     SCT    P VAR? HAOMHAET EPEMEHHE TA RV TAU: P
              BOEH EPOA OHAPBAETC MEHEHE BCO-
              T MAX I  H MIN II./RESEMBLES RV TAU TYPE
              VARIABLES: IF THE PERIOD IS DOUBLED, THE NEIGHT OF
              MAX I AND THE DEPTH OF MIN II VARY.
CR     SCT    MIN II 12.1; DII=0.071P; MIN II-MIN I=0.53P.
CT     SCT    MIN II 11.1.
CW     SCT    MIN II 10.1.
CZ     SCT    CM./SEE V1389 SGR.
DD     SCT    OH  KOMOHEHTOB, O-BMOM, MEHET ECK./
              ONE OF THE COMPONENTS PROBABLY VARIES.
DE     SCT    MIN II 16.3.
DG     SCT    D=0.03P:.
DL     SCT    MIN II 15.9.
DT     SCT    MIN II 16.5.
DV     SCT    MIN II 17.8.
DW     SCT    MIN II 16.4.
EE     SCT    MIN II 15.3.
EH     SCT    MIN II 15.0.
EK     SCT    MIN II 16.0.
EL     SCT    OPMA KPBO ECKA MEHETC?/THE SHAPE OF THE
              LIGHT CURVE VARIES?
EN     SCT    MIN II 17.2. BOMOH TAKE PE EMEHT:/
              THE DIFFERENT ELEMENTS ARE ALSO POSSIBLE:
              MIN I=2428008.85+1.06446D*E.
EP     SCT    D=0.04P:; MIN II 15.6.
EQ     SCT    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6631.
              MIN II 12.6:.
ER     SCT    MIN II 9.3; MIN II-MIN I=0.506P; DII=0.14P.
EU     SCT    VB A (B 17.5M, 6", 45G).
EV     SCT     A/H!=-0.4. EH PACCEHHOO CKOEH/THE MEM-
              BER OF THE OPEN CLUSTER NGC 6664.
EW     SCT    P0=5.8195D (A/2=0.27M), P1=4.0646D (A/2=0.22M);
              P1/P0=0.6984.
EX     SCT    D=0.025P:.
EY     SCT    MIN II 12.4. B OACT PACCEHHOO CKOEH/IN
              THE REGION OF THE OPEN CLUSTER NGC 6683.
EZ     SCT    MIN II 12.5.
FF     SCT    MIN II 14.2.
FG     SCT    MIN II 14.70. P VAR? MIN I=2429017.557+
              +0.2705728D*E (J.D.2427975-29520)  1397!; OCE/
              SINCE J.D.2444700-CM.TA./SEE TABLE.
FH     SCT    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6694.
FK     SCT    MIN II 14.4:.
FL     SCT    MIN II 13.8.
FM     SCT    MIN II 12.9.
FN     SCT    B PACCEHHOM CKOEH/IN THE OPEN CLUSTER
              NGC 6704.
FO     SCT    D=0.22D.
FR     SCT    OCAHE CEKTPA/SPECTRUM DESCRIPTION  1410!.
GI     SCT    MIN II 14.5.
GM     SCT    MIN II 13.8:.
HI     SCT    D=0.29D.
HL     SCT    MIN II 13.4.
IS     SCT    P<200D.
IT     SCT    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6705.
LL     SCT    SF KOMOHEHT TECHO BOHO CCTEM./SF COMPO-
              NENT OF A CLOSE PAIR.
LR     SCT    B PAOHE APOBOO CKOEH/IN THE REGION OF THE
              GLOBULAR CLUSTER NGC 6712.
LU     SCT    P2=30D.
LZ     SCT    CM./SEE LR SCT.
MM     SCT    MIN II 15.8.
MP     SCT    V1 (NGC 6712). EH TOO APOBOO CKOEH./
              THE MEMBER OF THIS GLOBULAR CLUSTER.
               FE/H!=-0.69.
MR     SCT    V8 (NGC 6712). P VAR. MAX=2430885+117D*E
              (J.D.2427900-32400)  4231!; OCE/SINCE
              J.D.2434900-CM.TA./SEE TABLE.
NU     SCT    VB A (B 16.6M, 12", 180G).
NV     SCT    P=200D?
OU     SCT    P VAR. MAX=2427620+152D*E (J.D.2426200-32800);
              OCE/SINCE J.D.2433100-CM.TA./SEE TABLE.
PT     SCT    MEETC K CTHK 16.4M./THERE IS A CLOSE
              COMPANION, 16.4M.
PW     SCT    AH PEE MEHEH CMMAPHOO ECKA EPE-
              MEHHO  KOO CTHKA, CEEO A HE./
              THE RANGE OF THE COMBINED LIGHT OF THE VARIABLE AND
              A CLOSE COMPANION, WHICH FOLLOWS, IS GIVEN IN THE
              TABLE.
QU     SCT    EPEMEHHA BETC TAKE ATMEHHO C P=0.2D 
              A=0.7M./THE VARIABLE IS ALSO ECLIPSING ONE WITH
              P=0.2D AND A=0.7M.
V337   SCT    K CTHK/A CLOSE COMPANION (16.2M, <7",
              90G).
V340   SCT    MIN II 15.6.
V356   SCT    MIN II 12.3; DII=0.10P.
V360   SCT    K FN CTHK 16.4M./A CLOSE FN COMPANION,
              16.4M.
V362   SCT    P=170D?
V367   SCT    B PACCEHHOM CKOEH/IN THE OPEN CLUSTER
              NGC 6649.
              B TAE AH EMEHT KOEAH C OCHOBHM
              EPOOM P0 (A0=0.54M B).  EPOA EPBOO
              OEPTOHA P1 (A1=0.41M B) MAX=2437435.12+
               +4.38466D*E; P1/P0=0.696744./THE LIGHT ELEMENTS
              WITH FUNDAMENTAL MODE PERIOD P0 (A0=0.54M B) ARE
              GIVEN IN THE TABLE. FOR THE FIRST-OVERTONE PERIOD
              P1 (A1=0.41M B) MAX=2437435.12+4.38466D*E;
              P1/P0=0.696744.
              M-M VAR (0.15<=M-M<=0.45).
V369   SCT    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6705 (M 11).
              HAAETC HAOEHE ETPEX EPOOB KOEA-
              H ECKA:/THERE IS A SUPERPOSITION OF THE FOUR
              LIGHT OSCILLATIONS: P1=0.240D (A1=0.044M), P2=0.220D
              (A2=0.020M), P3=0.182D (A3=0.068M), P4=0.114D
              (A4=0.028M)  9745!.
V370   SCT    D=0.016P.
V372   SCT    D=0.012P.
V414   SCT    OO CTHK?/BLUE COMPANION?
DELTA  SCT    VB A (B 10M, 53", 130G); (K-B)2=0.37.
              HA OCHOBHOE KOEAHE C EPOOM P0 (A0=0.125M),
              PBEEHHM B TAE, HAKABAETC BTOPOE C
              EPOOM P1=0.1867756D (A1=0.034M)  9975!.
R      SER    P VAR. MAX=2372429+356.93D*E (J.D.2372400-
              88900)  0960!; MAX=2397809+353.00D*E
              (J.D.2394000-2403000); MAX=2403104+357.25D*E
              (J.D.2403000-24000); MAX=2432387+356.10D*E
              (J.D.2424000-39200); OCE/SINCE J.D.2441000-
              CM.TA./SEE TABLE.
              MAEP/MASER (SIO, H2O).
S      SER    P VAR. MAX=2394360+361.01D*E (J.D.2394000-
              2407000); MAX=2407024+372.70D*E (J.D.2407000-
              17000)  0960!; MAX=2425875+366.59D*E
              (J.D.2417000-36000); OCE/SINCE J.D.2437600-
              CM.TA./SEE TABLE.
              MAEP/MASER (OH, SIO, H2O).
T      SER    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6633.
              P VAR. MAX=2400907+342.05D*E (J.D.2400500-
              15000); MAX=2417912+345.73D*E (J.D.2417900-
              26000); MAX=2428524+332.21D*E (J.D.2426000-
              32500); MAX=2438382+345.71D*E (J.D.2432500-
              39500); OCE/SINCE J.D.2439500-CM.TA./SEE
              TABLE.
              0.8' OT/FROM BN SER.
U      SER    P VAR. MAX=2421158+237.70D*E (J.D.2414000-
              22000); MAX=2422347+236.78D*E (J.D.2422000-
              26600); MAX=2426609+239.21D*E (J.D.2426600-
              32500); OCE/SINCE J.D.2432500-CM.TA./SEE
              TABLE.
V      SER    MIN II 9.85.
W      SER    P VAR, HEHEHE EH/NONLINEAR TERMS:
              +(3.140D*10**-6)*E**2+(1.432D*10**-9)*E**3.
              OPMA KPBO ECKA VAR. BOHOOPAHE KOEA-
              H B MAX. MEHEH MCCOHHX H C OP-
              TAHO AO. AKTBH OMEH MACCO, PHAK
              OE OOOK./THE LIGHT CURVE SHAPE VAR. WAVE-
              LIKE VARIATIONS IN MAX LIGHT. CHANGES OF EMISSION
              LINES WITH THE ORBITAL PHASE. ACTIVE MASS EXCHANGE,
              EVIDENCE FOR A COMMON ENVELOPE.
X      SER    OCE 1932 OTMEAC KOEAH ECKA 14.3M-
              18.3M; COACHO  1417!, P=275D. O HAEHM
              1961-1964 P=275D HE OTBEPEH, AOOPEH
              KTA ECKA C EPOOM HECKOKO MHT
               3625!./AFTER 1932 VARIATIONS 14.3M-18.3M WERE NO-
              TED; ACCORDING TO  1417!, P=275D. OBSERVATIONS IN
              1961-1964 DID NOT CONFIRM P=275D, FLUCTUATIONS OF
              LIGHT WITH A PERIOD OF SEVERAL MINUTES WERE SUSPECTED
               3625!.
              CEKTPAHE AHHE OTHOCTC K 1981 ./THE
              SPECTRAL DATA ARE FOR 1981.
Y      SER    AHA OXA MIN. COACHO  8643!, HA KOEAH C
              P-400D HAKABAETC P-40D./EPOCH OF MIN IS
              GIVEN. ACCORDING TO  8643!, VARIATIONS WITH P-400D
              ARE SUPERIMPOSED BY P-40D.
Z      SER    EMEHT PAOTAT B HTEPBAE/THE ELEMENTS ARE
              VALID DURING J.D.2422000-31000.
RS     SER    MIN II 11.4.
RT     SER    MAX (1920-1923).
              B CEKTPE (1977-1979) MCC/IN THE SPECTRUM
              (1977-1979) THERE ARE EMISSIONS HALFA-HDELTA, HEI, HEII,
               OI!  P./ETC. ACOP/ABSORPTIONS TIO.
RV     SER    MAEP/MASER (H2O).
VY     SER     FE/H!=-1.77, DS=9.
WW     SER    MAEP/MASER (H2O).
WX     SER    MAEP/MASER (OH, SIO, H2O). P VAR?
AA     SER     A/H!=0.2.
AG     SER    P VAR? OCE/SINCE J.D.2435000-CM.TA./SEE
              TABLE.
AK     SER    P VAR? O/BEFORE J.D.2442300 MIN=2431313.266+
              +1.9225667D*E  0318!; OCE/SINCE J.D.2442300-
              CM.TA./SEE TABLE.
AN     SER    P VAR? MAX=2429156.260+0.5220703D*E
              (J.D.2427000-38000)  0001!; OCE/SINCE
              J.D.2438000-CM.TA./SEE TABLE.
              COACHO  2740!, EKT AKO C =21.94D; B
               7258! HAE EKTA AKO OTPAETC./
              ACCORDING TO  2740!, BLAZHKO EFFECT WITH =21.94D;
              THE PRESENCE OF THE BLAZHKO EFFECT IS DENIED IN
               7258!.
              DS=0.
AO     SER    MIN II 10.8.
AP     SER    VB A (B 14.29M, 8" SP).  FE/H!=-1.37.
AQ     SER    MIN II 11.1.
AR     SER    P VAR. O/BEFORE J.D.2425000 MAX=2415617.698+
              +0.5752221D*E; MAX=2425313.530+0.57508945D*E
              (J.D.2425000-28500); MAX=2428848.662+
              +0.575214D*E (J.D.2428500-31000)  8081!; MAX=
              =2431436.424+0.5751134D*E (J.D.2431000-34200);
              MAX=2436013.279+0.5752169D*E (J.D.2435900-
              37200); MAX=2438138.467+0.5750651D*E
              (J.D.2437200-38700)  0001!. PAOTAE B CPEHEM
              EMEHT OCE/ELEMENTS WORKING ON AVERAGE SINCE
              J.D.2438700-CM.TA./SEE TABLE.
              COH EKT AKO./COMPLEX BLAZHKO EFFECT.
              =108.4D  8082!. A VAR (0.23M-0.87M V).  VAR (80D-
              120D)  7032!.
              DS=4.6.
AS     SER    MIN II 11.5.
              MOMEHT MIN I 2442937.428 (BBSAG) HE OBETBOP-
              ETC EMEHTAM./THE EPOCH OF MIN I 2442937.428
              (BBSAG) IS NOT IN AGREEMENT WITH THE ELEMENTS.
AT     SER    P VAR. MAX=2415353.783+0.74655695D*E
              (J.D.2415000-27000); MAX=2428337.260+
              +0.7465670D*E (J.D.2428000-39500); OCE/SINCE
              J.D.2441500-CM.TA./SEE TABLE.
              DS=9.
AU     SER    MIN II 11.61.
              OPMA KPBO ECKA/THE LIGHT CURVE SHAPE VAR.
AV     SER    DS=6.
AW     SER    DS=5.0.
BF     SER     A/H!=-2.5. DS=6.
BH     SER    P VAR. MAX=2427956.674+0.434545D*E (J.D.2425000-
              30700)  1039!; OCE/SINCE J.D.2437650-CM.TA./
              SEE TABLE.
BI     SER    MIN I 2446264.414  10200! POTBOPET EMEH-
              TAM/CONTRADICTS THE ELEMENTS. P VAR?
BN     SER    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6633. 0.8' OT/FROM T SER.
BO     SER    P VAR? MAX=2425681+201D (J.D.2425600-30100)
               0447!; B TAE AH CPEHE EMEHT/THE
              TABLE GIVES MEAN ELEMENTS (J.D.2425600-35400).
BQ     SER    P0-CM.TA./SEE TABLE. P1=3.012D  8188!.
              CM./SEE BR SER.
BR_BU  SER    B OACT PACCEHHOO CKOEH/IN THE REGION
              OF THE OPEN CLUSTER IC 4756.
CC     SER    MIN II 11.63.
CN     SER     FE/H!=-0.77. DS=3.4.
CO     SER    P VAR? OPMA KPBO ECKA/THE LIGHT CURVE SHAPE
              VAR.
               FE/H!=-1.38. DS=7.2.
CQ     SER    MIN II 12.0.
CR     SER     A/H!=-0.2.
CS     SER    P VAR. MAX=2418137.875+0.5267904D*E
              (J.D.2416000-32500)  0001!; OCE/SINCE
              J.D.2432500-CM.TA./SEE TABLE.
              DS=(6).
CV     SER    B OACT HII-KOMEKCA S 54  PACCEHHOO
              BEHOO CKOEH NGC 6604. CBAHA C TMAH-
              HOCT OOOEHO CTPKTP.
              HOA HAATC ATMEH B KOHPA
              "WR BEPE O" (CM.TA.), HOA-B KOH-
              PA "O BEPE WR", KOTOPO COOTBETCTBOBAO
              HAOEE OKOE HAABEEC ATMEHE (-
              HO 0.5M B, V). BPEMEHAM OTOMETPECKOE
              ATMEHE B EMEPHE MOMEHT OTCTCTBET, 
              HAAETC  ATMOCEPHOE ATMEHE O-BE-
               WR-KOMOHEHTOM B LAMBDA 4653 A (MCC CII-CIV,
              NIII), LAMBDA<2000 A. K-TOK; BOMOHO K-
              ATMEHE B KOHPA "O  BEPE WR"./
              IN THE REGION OF THE HII COMPLEX S 54 AND THE OPEN
              STAR CLUSTER NGC 6604. CONNECTED WITH A SHELL-STRUC-
              TURE NEBULA.
              SOMETIMES ECLIPSES ARE OBSERVED DURING THE CONFIGU-
              RATION "WR IN FRONT OF O" (SEE TABLE) AND SOMETIMES
              DURING THE CONFIGURATION "O IN FRONT OF WR" WHICH
              COINCIDED WITH THE DEEPEST ECLIPSE EVER OBSERVED
              (WITH THE DEPTH 0.5M B, V). SOMETIMES THE PHOTOMET-
              RIC ECLIPSE AT PREDICTED MOMENTS DOES NOT OCCUR, AND
              ONLY THE ATMOSPHERIC ECLIPSE OF THE O STAR WITH THE
              WR COMPONENT IS OBSERVED AT LAMBDA 4653 A (EMISSION OF
              CII-CIV, NIII), LAMBDA<2000 A. IR EXCESS; POSSIBLY AN
              IR ECLIPSE IN THE CONFIGURATION "O  IN FRONT OF WR".
CX     SER    HA KPBO ECKA (HAOMHAE ATMEHH KP-
              B ECKA U GEM) OP BCOTO-0.2M, PEE-
              CTB MHMM; KTA ECKA B MAX O
              -0.3M-0.4M./THE LIGHT CURVE (RESEMBLING THE ECLIP-
              SING LIGHT CURVE OF U GEM) SHOWS A HUMP OF-0.2M
              HEIGHT BEFORE THE MINIMUM; FLUCTUATIONS UP TO-0.3M-
              0.4M IN MAX.
DF     SER    VB A (B 13.9M, 0.4', -115G).
DG     SER    MIN II 16.5:. BOMOEH COPEHH EPO/THE
              ALIAS PERIOD IS POSSIBLE (0.3360742D).
DH     SER    PO BOMOH P/ANOTHER POSSIBLE P=450D.
DK     SER    MAX 2433829  10008! POTBOPET EMEHTAM/
              CONTRADICTS THE ELEMENTS.
DR     SER    VB A (B 12.54M, 28", 0G).
DT     SER    VB A (B-5").
              B CEKTPE MCC/THE SPECTRUM SHOWS EMISSIONS
              OF  OIII! LAMBDA LAMBDA 4959, 5007 A.                     O-
CMOTECKA?/SYMBI
              TIC?  8676!.
DV     SER    B HEOOM BEHOM CKOEH./IN A SMALL STAR
              CLUSTER.
DY     SER     FE/H!=-1.58. DS=8.4.
EE_EF  SER    B OACT PACCEHHOO CKOEH/IN THE REGION
              OF THE OPEN CLUSTER M 17=NGC 6618.
EG     SER    VB A (RO>10").
EL     SER    N<=7.
EN     SER     FE/H!=-1.07. DS=5.3.
EO     SER    OO PAPOC HA KPBO ECKA. BOMOEH T
              RR(B)./THE LIGHT CURVE SHOWS LARGE SCATTER. RR(B)
              TYPE IS POSSIBLE.
              MAX=2437433.653+0.6309D*E (J.D.2437433-514)
               3625!.
               FE/H!=-1.63. DS=8.8.
ER_ET  SER    B OACT PACCEHHOO CKOEH/IN THE REGI-
              ON OF THE OPEN CLUSTER M 16=NGC 6611.
EU     SER    VB A (B 4" NP). EH PACCEHHOO CKOEH/
              A MEMBER OF THE OPEN CLUSTER M 16=NGC 6611.
              K TOK/IR EXCESS.
EV_EX  SER    CM./SEE ER SER.
FI     SER    EPOHOCT HAMEAETC B AX U./HINTS OF
              PERIODICITY IN U LIGHT.
FK     SER    VB (DM-0.5M, 1.3", 11.5G, 1972).
              B AATMOCEPHOM TPAOETE APECTPPOBA-
              H BCK  10013!. OTMEATC OT OT XA-
              PAKTEPHX BE TA BY  BEPOTHA PHAE-
              HOCT K CTA "OCE T TAU"  7260, 3866!./FLARES
              WERE FOUND IN THE SATELLITE UV RANGE  10013!. DIFFE-
              RENCES FROM TYPICAL BY STARS AND PROBABLE "POST-
              T TAU" NATURE ARE NOTED  7260, 3866!.
              COACHO/ACCORDING TO  6948!, MIN=2441939.200+
              +5.20D*E.
              MK PEHTEHOBCK CTOHK./SOFT X-RAY SOURCE.
FL     SER    VB (DM=1.9M, 0.46", 145G, 1981).
FM     SER    CM./SEE ER SER.
              VB (VAR SF?).
FN     SER    CM./SEE ER SER.
FR     SER    ADS 11477 A (B 12.5M, 10.5", 330G, 1924; C 9.3M,
              30.5", 5G, 1930).
              BOMOHE HAEH P:/POSSIBLE VALUES OF P:
              2.1308D, 2.1565D.
LN     SER    MPQ=17.5M=CONST; OO CTHK? BLUE COMPA-
              NION?  7264!.
LS     SER    OOE PACCEHE HA KPBO ECKA, EMEHT
              HATC B OTBEPEH./THE LIGHT CURVE SHOWS
              LARGE SCATTER, THE ELEMENTS NEED CONFIRMATION.
              BOMOHA EHTKA C PEHTEHOBCKM CTO-
              HKOM/POSSIBLE IDENTIFICATION WITH AN X-RAY SOURCE
              2ASE 1822+0.
LV     SER    AHA OXA MAX B AX V; B B  U MEHEH B
              POTBOAE./THE EPOCH OF MAX IN V LIGHT IS GIVEN;
              IN B AND U VARIES IN OPPOSITE PHASE.
LX     SER    HA ATMEH/THE DEPTH OF ECLIPSES-2.5M.
              CPABHTEHO ACTE BCK/COMPARATIVELY FRE-
              QUENT OUTBURSTS  10023!.
MM     SER    SER X-1=4 U 1 837+04. LX/LOPT>=100.
              VB B (A 19.1M; B 2.2", 210G).
MO     SER    V1 (NGC 6535). HE EH CKOEH./CLUSTER NON-
              MEMBER.
MP     SER    V2 (NGC 6535). HE EH CKOEH./CLUSTER NON-
              MEMBER.
DELTA  SER    ADS 9701A (B 5.16M, DF0, A=5.843", PORB=3168 YR;
              4", 175G, 1980).
OMIKRO SER    SB?
D      SER    ADS 11353 A (B 7.44M, SB?, F5V, 3.9", 320G, 1983).
              VB (CEK-HTEPEPOMETPECKA/SPECKLE-INTERFE-
              ROMETRIC; 0.25", 157G, 1976). SB (P1ORB=385D,
              P2ORB=1.8505205D).
S      SEX    P VAR. MAX=2422029+257.2D*E (J.D.2417650-22050);
              MAX=2428968+266.65D*E (J.D.2422050-30300); MAX=
              =2434739+260.86D*E (J.D.2430300-34750); MAX=
              =2438796+254.3D*E (J.D.2434750-38800); OCE/
              SINCE J.D.2440600-CM.TA./SEE TABLE.
T      SEX     FE/H!=-1.20. P VAR. MAX=2416146.675+
              +0.32465971D*E (J.D.2414000-18300), MAX=
              =2424561.398+0.32467107D*E (J.D.2418300-24570)
               0752!; MAX=2424561.430+0.3246702D*E
              (J.D.2424560-28280), MAX=2429350.320+
              +0.3247113D*E (J.D.2429350-34370), MAX=
              =2434795.409+0.3246978D*E (J.D.2434795-36630)
               9978!; OCE/SINCE J.D.2441380-CM.TA./SEE
              TABLE.
U      SEX    P VAR. MAX=2419823.355+0.53402622D*E
              (J.D.2419470-36670)  3697!; OCE/SINCE
              J.D.2443980-CM.TA./SEE TABLE.
Y      SEX    MIN II 10.17; DII=0.05P. P VAR. MIN I=2428122.700+
              +0.41982341D*E (J.D.<2429000)  0007!; MIN I=
              =2434445.989+0.419818D*E (J.D.2428100-35000)
               0001!, MIN I=2439521.964+0.41981543D*E
              (J.D.2431150-43250)  9981!; OCE/SINCE
              J.D.2440300-CM.TA./SEE TABLE.
RU     SEX    MIN II 11.4. COACHO/ACCORDING TO  9923!, RR?
              (P=0.5398D?), CEP? (P=6.792D?).
RW     SEX    PORB=0.247D  9925!; LX/LOPT=10**-4  9926!;
              PX=254S  9927!.
RX     SEX    VB A (B 9.1M, 116.3", 191G).
RY     SEX    MU=0.67", P=281G.
R      TAU    OH, H2O, SIO MAEP/MASER. P VAR. MAX=2411012+
              +325.0D*E (J.D.2398654-2414000); MAX=2424243+
              +322.1D*E (J.D.2414000-24300); MAX=2434005+
              +325.4D*E (J.D.2424300-35500); OCE/SINCE
              J.D.2435500-CM.TA./SEE TABLE.
S      TAU    P VAR. MAX=2404646+380.1D*E (J.D.2399326-
              2405000); MAX=2425085+371.40D*E (J.D.2405000-
              26000); OCE/SINCE J.D.2426000-CM.TA./SEE
              TABLE.
T      TAU    VB A (B 15M, 0.27", 358G; C-HPAKPACH CT-
              HK/INFRARED COMPANION, 0.590", 180G).
              POM C EPEMEHHO TMAHHOCT/NEAR THE VARIABLE
              NEBULA NGC 1555.
              OH, H2O MAEP/MASER.
              B HTEPBAE/IN THE INTERVAL J.D.2402140-21000 PE-
              E MEHEH ECKA/THE LIGHT RANGE 9.3M-13.5M,
              OCE/SINCE J.D.2421000-/ONLY 9.5M-10.8M.
U      TAU    VB (A 10.9M; B 12.0M, 3", 77G).
V      TAU    P VAR. MAX=2417978+170.0D*E (J.D.2404550-18000);
              MAX=2424580+169.3D*E (J.D.2418000-24600);
              MAX=2432746+170.1D*E (J.D.2424600-33500);
              MAX=2436970+168.7D*E (J.D.2433500-37300);
              MAX=2442442+171.1D*E (J.D.2437300-43000);
              OCE/SINCE J.D.2443000-CM.TA./SEE TABLE.
W      TAU    B TAE PBEEHO HAEHE <P>./<P> VALUE IS
              GIVEN IN THE TABLE.
              P VAR. MAX=2415320+274.1D*E (J.D.2410360-15500),
              MAX=2421995+266.1D*E (J.D.2415500-22500),
              MAX=2425135+260.5D*E (J.D.2422500-28800),
              MAX=2438837+245.4D*E (J.D.2428800-39100)  0001!.
Z      TAU    VB A (B 13.6M, 4", 45G).
              P VAR. MAX=2425115+499.90D*E (J.D.2415100-26500)
              MAX=2438768+486.20D*E (J.D.2426500-39000);
              OCE/SINCE J.D.2439000-CM.TA./SEE TABLE.
RR     TAU    OCAHE CEKTPA  OTO TMAHHOCT/SPECTRUM DES-
              CRIPTION AND THE PHOTOGRAPHS OF THE NEBULA  4002!.
RU     TAU    VB A (B 4"). P VAR. MAX=2426004+545.3D*E
              (J.D.2415009-27500). MAX=2434309+604.0D*E
              (J.D.2427500-34500); OCE/SINCE J.D.2437500-CM.
              TA./SEE TABLE.
RV     TAU    OH MAEP/MASER. CPEH ECK MEHETC/MEAN
              BRIGHTNESS VARIES: MIN=2417553+1224D*E  0580!.
RW     TAU    VB A (12.5M, 1.3", 172G, 1959). DI=0.020P; MIN II 8.09.
              P VAR. MIN I=2417198.410+2.7688665D*E+
              +0.038D SIN 0.0818G (E-100) (J.D.2409913-24150),
              MIN I=2434423.3571+2.7688209D*E (J.D.2424150-
              37000)  5460!; MIN I=2437164.4860+2.7688480D*E
              (J.D.2437000-39900)  7531!; MIN I=2442776.93772+
              +2.76884463D*E (J.D.2439855-42780)  8593!; MIN I=
              =2442776.9313+2.7688396D*E (J.D.2442780-45750)
               9084!; OCE/SINCE J.D.2445750-CM.TA./SEE
              TABLE.
              OPMA KPBO ECKA MEHETC./THE SHAPE OF THE
              LIGHT CURVE VARIES.
RX     TAU    OH, H2O MAEP/MASER.
              P VAR. MAX=2423561+338.4D*E (J.D.2417155-24000);
              MAX=2430505+330.2D*E (J.D.2424000-30700); MAX=
              =2437963+339.3D*E (J.D.2430700-38000); OCE/
              SINCE J.D.2438000-CM.TA./SEE TABLE.
RY     TAU    SB 1. OTO TMAHHOCT  OCAHE CEKTPA/THE PHO-
              TOGRAPHS OF THE NEBULA AND SPECTRUM DESCRIPTION
               5064!. BOMOH OOEPOECKE KOEAH
              ECKA C KAM 70.25, 15.9, 9.4  5.84 OA/LONG
              PERIOD LIGHT VARIATIONS ARE POSSIBLE WITH CYCLES
              70.25, 15.9, 9.4 AND 5.84 YEARS  9993!.
RZ     TAU    MIN II 10.66. P VAR. MIN I=2424032.1426+
              +0.41567109D*E (J.D.2424000-34100)  0312!; OCE/
              SINCE J.D.2436000-CM.TA./SEE TABLE.
SS     TAU    P VAR  3506!. MAX=2420894.2339+0.3699665D*E (J.D.
              2420890-21300)  9995!; MAX=2426669.080+
              +0.3699687D*E (J.D.2426400-26700)  0320!; MAX=
              =2428843.856+0.3699231D*E (J.D.2426700-30300),
              MAX=2431392.603+0.369912D*E (J.D.2430300-31400),
              MAX=2432118.794+0.369937D*E (J.D.2431400-32150),
              MAX=2432857.884+0.3699146D*E (J.D.2432150-35000),
              MAX=2435055.528+0.3699066D*E (J.D.2435000-36400),
              MAX=2437313.503+0.3699266D*E (J.D.2436400-37320),
              MAX=2437960.419+0.369878D*E (J.D.2437300-37960),
              MAX=2437960.419+0.369938D*E (J.D.2437960-38740);
              OCE/SINCE J.D.2438740-CM.TA./SEE TABLE.
SV     TAU    MIN II 9.8.
SW     TAU    P VAR. MAX=2432049.856+1.583623D*E (J.D.2418240-
              36000); OCE/SINCE J.D.2436000-CM.TA./SEE
              TABLE.
SX     TAU    B PAOHE CKOEH E. HE EH CKOEH./
              IN THE REGION OF THE PLEIADES CLUSTER. NOT A MEMBER
              OF THE CLUSTER.
SY     TAU    CM./SEE SX TAU.
SZ     TAU    EH KOPOH PACCEHHOO CKOEH/THE MEMBER
              OF THE HALO OF THE OPEN CLUSTER NGC 1647.
              P VAR. MAX=2410000.60+3.1487D*E (J.D.2412000-
              20200)  9996!; MAX=2419267.519+3.149046D*E
              (J.D.2419260-34650); OCE/SINCE J.D.2434650-
              CM.TA./SEE TABLE.
TT     TAU    P=364D?  0589!.
TY     TAU    B PAOHE CKOEH A. HE EH CKOEH./IN
              THE REGION OF THE HYADES CLUSTER. NOT A MEMBER OF
              THE CLUSTER.
              COACHO/ACCORDING TO  9997!, MIN=2422291.303+
              +0.539250D*E.
UU     TAU    CM./SEE SX TAU.
UX     TAU    VB A (B 13.67M V, M2.5 VE, 5.74", 270.1G, 1944).
UZ     TAU    VB A (B 15.16M B, M4VE (LI), 3.7", 271.5G, 1944).
              B TAE AH PEE MEHEH CMMAPHOO
              ECKA./THE RANGE OF THE COMBINED LIGHT VARIATION IS
              GIVEN IN THE TABLE.
WW     TAU    P VAR. P=114.8D (J.D.2414800-20800). P=124.4D
              (J.D.2420800-23700)  0634!; P=114D (J.D.2424800-
              26300), P=139D (J.D.2426300-27700)  0310!; P=
              =114D (J.D.2427900-30800), P=131D (J.D.2430800-
              31500), P=109D (J.D.2431500-33400)  0364!;
              OCE/SINCE J.D.2433400-CM.TA./SEE TABLE.
WY     TAU    MIN II 11.73. P VAR?  10048!.
WZ     TAU    VB.
XZ     TAU    VB A (B=HL TAU, 23", 273G).
YZ     TAU     FE/H!=-1.53. CM./SEE SX TAU.
              EMEHT COEPAT KBAPATH EH:/THERE IS A
              SQUARE TERM IN THE ELEMENTS:-6D*10**-11*E**2.
AA     TAU    BOMOHA KHOCT MEHEH ECKA C P=4.5D
               2D  10003!, A TAKE 8.2D  10004!./CYCLIC LIGHT VARI-
              ATION WITH P=4.5D AND 2D  10003! AND ALSO 8.2D  10004!
              IS POSSIBLE.
AC     TAU    D=0.025P. P VAR?
AH     TAU    MIN II 11.85. P VAR? CM./SEE SX TAU.
AL     TAU    P VAR. HA MIN II/THE DEPTH OF MIN II 0.15M.
AM     TAU    D=0.012P:. P VAR. MIN I=2427534.444+2.044018D*E
              (J.D.2425580-27540), MIN I=2435019.436+
              +2.043935D*E (J.D.2433320-37020); OCE/SINCE
              J.D.2442365-CM.TA./SEE TABLE.
AN     TAU    MIN II 10.5; MIN II-MIN I=0.53P. P VAR.
AP     TAU    MIN II 14.7; MIN II-MIN I=0.48P.
AS     TAU    P VAR. MIN I=2439390.595+3.4835542D*E (J.D.
              2419440-44300)  7806!; OCE/SINCE J.D.2444300-
              CM.TA./SEE TABLE.
AU     TAU    P VAR. MAX=2426642+71.0D*E (J.D.2426290-30400)
               0310!; OCE/SINCE J.D.2438000-CM.TA./SEE
              TABLE.
AW     TAU    OH, H2O MAEP/MASER.
              P VAR. MAX=2426278+690D*E (J.D.2416100-33850)
               0609!; OCE/SINCE J.D.2433850-CM.TA./SEE
              TABLE.
BB     TAU    SC 7/7 E.
BK     TAU    CM./SEE SX TAU.
BN     TAU    P VAR. MIN I=2435460.370+4.2542044D*E (J.D.
              2419000-39100)  5466!; OCE/SINCE J.D.2443000-
              CM.TA./SEE TABLE.
BP     TAU    HAATC KBACHCOAHE KOEAH EC-
              KA C P=7.6D/THERE ARE QUASISINUSOIDAL LIGHT VARIA-
              TIONS WITH P=7.6D  10011!.
BU     TAU    SB? EOHA. EH CKOEH E./PLEIONE.
              THE MEMBER OF THE PLEIADES CLUSTER.
BV     TAU    MIN II 11.9.
BW     TAU    3C 120. CEEPTOBCKA AAKTKA/SEYFERT GALAXY;
              Z=0.033.
              OCAHE CEKTPA/SPECTRUM DESCRIPTION  10012!.
CD     TAU    VB A (B 9.88M, 9.9", 148.8G). MIN II 7.31.
              B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER CR 65.
CF     TAU    D=0.02P; MIN II 10.2;
CH     TAU    CM./SEE V1389 SGR.
CM     TAU    SN 1054 B KPAOBHO TMAHHOCT/IN THE CRAB NE-
              BULA (NGC 1952=M1); CAP/PULSAR NP 0532.
              OXA BCK/THE OUTBURST EPOCH IS J.D.2106210:.
              EHE CAPA MEHETC OHOBPEMEHHO BO
              BCEM AAOHE H BOH-OT GAMMA-E O PAO-
              BOH C P=0.033S B PEEAX 13.9M-17.7M V./THE PUL-
              SED RADIATION VARIES PRECISELY IN PHASE OVER THE WHO-
              LE SPECTRUM, FROM RADIO WAVES TO GAMMA RAYS WITH
              P=0.033S IN THE RANGE 13.9M-17.7M V.
              P VAR  10017, 10018!: 0.033095563927S
              (J.D.2440297.5094)<=P<=0.033242051159S
              (J.D.2444312.750).
CR     TAU    P=1.362692D?
CT     TAU    MIN II 11.12. P VAR. MIN I=2437312.369+0.6668274D*E
              (J.D.2432700-38790)  10010!; OCE/SINCE
              J.D.2441400-CM.TA./SEE TABLE.
CU     TAU    CM./SEE SX TAU. MIN II 11.90. P VAR. MIN I=
              =2431822.5193+0.4126022D*E (J.D.2431060-2890)
               0604!; OCE/SINCE J.D.2440960-CM.TA./SEE
              TABLE.
CZ     TAU    VB B (A=DD TAU; B 31", 13G).
DD     TAU    VB A (B=CZ TAU; 31", 13G).
DE     TAU    VB A (B 26", 10G).
DG     TAU    CBAHA C HEOO PKO OOPAHO TMAHHO-
              CT./CONNECTED WITH A SMALL BRIGHT ARC-SHAPED NE-
              BULA.
DH     TAU    VB A (B=DI TAU, 16", 125G). COACHO  10004!,
              HAAETC EPOECKA EPEMEHHOCT ECKA C
              P=7.0D  A=0.4M V./ACCORDING TO  10004! THERE IS
              PERIODICAL LIGHT VARIABILITY WITH P=7.0D AND A=0.4M V.
DI     TAU    VB B (A=DH TAU; B 16", 125G). COACHO  10004!,
              HAAETC EPOECKA EPEMEHHOCT ECKA C
              P=7.7D  A<0.4M V./ACCORDING TO  10004! THERE IS
              PERIODICAL LIGHT VARIABILITY WITH P=7.7D AND A<0.4M V.
DL     TAU    VB A (B 17M V, 12", 333G). HAAETC K-
              HOCT MEHEH ECKA C P=2.7D  10003!./CYCLIC
              LIGHT VARIATION WITH P=2.7D IS PRESENT  10003!.
DN     TAU    HAATC CHCOAHE KOEAH ECKA C
              P=6.6D/THERE ARE SINUSOIDAL LIGHT VARIATIONS WITH
              P=6.6D  10011!.
DO     TAU    CM./SEE DG TAU.
DS     TAU    VB A (B 13.7M, 4", 288G). B TAE AH PEE
              MEHEH CMMAPHOO ECKA CCTEM./RANGE OF
              COMBINED LIGHT VARIATION OF THE PAIR IS GIVEN IN THE
              TABLE.
EI     TAU    VB?
EQ     TAU    MIN II 10.97. CM./SEE SX TAU.
ES     TAU    MIN II 14.4; MIN II-MIN I=0.52P; D=0.005P.
ET     TAU    MIN II 9.3.
EY     TAU    EH CKOEH A./THE MEMBER OF THE HYADES
              CLUSTER.
EZ     TAU    CM./SEE EY TAU.
FH     TAU    CM./SEE EY TAU.
FL     TAU    EH CKOEH E./THE MEMBER OF THE PLEIA-
              DES CLUSTER.
FS     TAU    VB A (B 16", 289G).
FV     TAU    VB A (B 13", 103G).
FW     TAU    VB A (B 13", 243G).
FY     TAU    VB B (A=FZ TAU, B 17", 250G).
FZ     TAU    VB A (B=FY TAU, 17", 250G).
GG     TAU    VB A (B 18.5M, 12", 205G).
GH     TAU    VB B (A=V807 TAU; B 21.4", 193G).
GI     TAU    VB B (A=GK TAU; B 13", 329G). HAATC KBA-
              CHCOAHE MEHEH ECKA C P=7.2D/
              THERE ARE QUASISINUSOIDAL LIGHT VARIATIONS WITH P=
              =7.2D  10011!.
              CM./SEE DG TAU.
GK     TAU    VB A (B=GI TAU, 13", 329G). HAATC KBA-
              CHCOAHE MEHEH ECKA C P=4.6D/THERE
              ARE QUASISINUSOIDAL LIGHT VARIATIONS WITH P=4.6D
               10011!.
              CM./SEE DG TAU.
GL     TAU    EHTPAHA BEA AHETAPHO TMAHHOCT/THE
              CENTRAL STAR OF THE PLANETARY NEBULA PK 174-14G1.
GP     TAU    P2=1000D.
GR     TAU    DI=0.068P; MIN II 10.49; MIN II-MIN I=0.516P.
GS     TAU    SB 1 (PORB=7.227424D  6568!). CM./SEE V1389 SGR.
GU     TAU    VB A (B 11", 299G).
GV     TAU    O'EKT XEPA-APO./HERBUG-HARO OBJECT.
GW     TAU    MIN II 11.7. P VAR?
GX     TAU    VB A (B 11", 310G).
HK     TAU    VB A (B 21M, 2", 180G).
HL     TAU    VB B (A=XZ TAU; B 23", 273G). CM./SEE DG TAU.
HN     TAU    VB A (B 18M, 3.3", 205G).
HO     TAU    VB A (B 8", 110G).
HP     TAU    CM./SEE DG TAU.
              COACHO  10004!, HAAETC EPOECKA EPE-
              MEHHOCT C P=1.2D./ACCORDING TO  10004! THERE IS PE-
              RIODICAL VARIABILITY WITH P=1.2D.
HR     TAU    VB B (A=HS TAU; B 14", 119G).
HS     TAU    VB A (B=HR TAU; 14", 119G).
HU     TAU    MIN II 5.91.
HZ     TAU    B PAOHE CKOEH E. BOMOH EH CKO-
              EH./IN THE REGION OF THE PLEIADES CLUSTER. POSSIBLE
              MEMBER OF THE CLUSTER.
II     TAU    B PAOHE CKOEH E. BOMOH EH CKO-
              EH A /IN THE REGION OF THE PLEIADES CLUSTER.
              POSSIBLE MEMBER OF THE HYADES CLUSTER
IK     TAU    OH, H2O, SIO MAEP/MASER.
IM     TAU    P VAR. MAX=2439792.398+0.144969D*E (J.D.2439790-
              43130)  10019!; P1=0.109016D, P1/P0=0.752. OCE/
              SINCE J.D.2444230-CM.TA./SEE TABLE.
IN     TAU    MU=0.121", P=105G. EH CKOEH A?/THE MEM-
              BER OF THE HYADES CLUSTER?
IO     TAU    B PAOHE CKOEH A/IN THE REGION OF THE HYA-
              DES CLUSTER.
IQ     TAU    VB A (B 17M, 11", 298G).
IS     TAU    C 1319  4051!. BEA N23 C MCCE B HALFA
               0596!. HA KAPTE OKPECTHOCTE, PBEEHHO B
               0596!, OOHO OOHAEHA HOMEPOM 26, B POTBO-
              PE C KOOPHATAM, PBEEHHM B TO E PAO-
              TE. TO PBEO K AHEM HEOPAMEHM P
              OTOECTBEH BE PM CCEOBATEM./
              THE STAR N23 WITH HALFA EMISSION  0596!. IN THE MAP GI-
              VEN IN  0596! ERRONEOUSLY DESIGNATED AS N26 IN CONT-
              RADICTION WITH THE CO-ORDINATES GIVEN IN THE SAME PA-
              PER. IT WAS THE REASON FOR DIFFERENT MISTAKES WHEN THE
              STAR WAS IDENTIFIED BY SOME OTHER INVESTIGATORS.
IT     TAU    C 1320  4051!. BEA N26 C MCCE B HALFA/
              THE STAR N26 WITH HALFA EMISSION  0596!.
              CM./SEE IS TAU.
KK     TAU    B PAOHE CKOEH E./IN THE REGION OF THE
              PLEIADES CLUSTER.
KL_KO  TAU    CM./SEE KK TAU.
KP     TAU    CM./SEE SX TAU.
KQ     TAU    CM./SEE KK TAU.
KR     TAU    CM./SEE SX TAU.
KS_KW  TAU    CM./SEE KK TAU.
KX     TAU    CM./SEE SX TAU.
KY     TAU    CM./SEE FL TAU.
KZ_LL  TAU    CM./SEE KK TAU.
LM     TAU    CM./SEE HZ TAU.
LN     TAU    CM./SEE KK TAU.
LO     TAU    CM./SEE HZ TAU.
LP     TAU    CM./SEE SX TAU.
LQ     TAU    CM./SEE KK TAU.
LR     TAU    CM./SEE II TAU.
LS     TAU    CM./SEE KK TAU.
LT_LV  TAU    CM./SEE HZ TAU.
LW     TAU    CM./SEE SX TAU.
LX     TAU    CM./SEE KK TAU.
LY     TAU    CM./SEE HZ TAU.
LZ_MM  TAU    CM./SEE FL TAU.
MN     TAU    CM./SEE KK TAU.
MO     TAU    CM./SEE HZ TAU.
MP_MQ  TAU    CM./SEE KK TAU.
MR_MS  TAU    CM./SEE FL TAU.
MT     TAU    CM./SEE SX TAU.
MU_MV  TAU    CM./SEE HZ TAU.
MW     TAU    CM./SEE KK TAU.
MX_MY  TAU    CM./SEE FL TAU.
MZ     TAU    CM./SEE HZ TAU.
NN_NO  TAU    CM./SEE KK TAU.
NP     TAU    CM./SEE FL TAU.
NQ     TAU    CM./SEE KK TAU.
NR     TAU    CM./SEE SX TAU.
NS     TAU    CM./SEE KK TAU.
NT     TAU    CM./SEE HZ TAU.
NU     TAU    CM./SEE KK TAU.
NV     TAU    CM./SEE SX TAU.
NW     TAU    CM./SEE KK TAU.
NX_NY  TAU    CM./SEE SX TAU.
NZ_OO  TAU    CM./SEE KK TAU.
OP     TAU    CM./SEE HZ TAU.
OQ     TAU    CM./SEE KK TAU.
OR_OT  TAU    CM./SEE FL TAU.
OU     TAU    MAX=2444896.758+0.39701D*E, M-M=0.5P, A(V)=
              =0.13M  10052!.
              CM./SEE FL TAU.
OW     TAU    CM./SEE FL TAU.
OX     TAU    CM./SEE KK TAU.
OY     TAU    CM./SEE SX TAU.
OZ_PP  TAU    CM./SEE HZ TAU.
PQ     TAU    CM./SEE SX TAU.
PR     TAU    CM./SEE FL TAU.
PS     TAU    CM./SEE KK TAU.
PT     TAU    CM./SEE FL TAU.
PU     TAU    CM./SEE KK TAU.
PV     TAU    CM./SEE HZ TAU.
PW_PZ  TAU    CM./SEE KK TAU.
QQ     TAU    SB2. CM./SEE FL TAU.
QR_QT  TAU    CM./SEE KK TAU.
QU     TAU    VB A (B 18.0M, 4.0", 135G). CM./SEE KK TAU.
QV_QW  TAU    CM./SEE KK TAU.
QX     TAU    CM./SEE FL TAU.
              MAX=2444896.79+0.483D*E, M-M=0.5P, A(V)=0.125M
               10052!.
QY     TAU    CM./SEE SX TAU.
QZ_    V335   TAU CM./SEE KK TAU.
V336   TAU    CM./SEE HZ TAU.
V337   TAU    CM./SEE KK TAU.
V338   TAU    CM./SEE HZ TAU.
V339   TAU    CM./SEE SX TAU.
V340_  V342   TAU CM./SEE KK TAU.
V343   TAU    CM./SEE FL TAU.
V344_  V345   TAU CM./SEE KK TAU.
V346   TAU    CM./SEE FL TAU.
V347   TAU    CM./SEE SX TAU.
V348   TAU    CM./SEE KK TAU.
V349_  V350   TAU CM./SEE HZ TAU.
V351   TAU    CM./SEE SX TAU.
V352   TAU    CM./SEE KK TAU.
V353_  V355   TAU CM./SEE HZ TAU.
V356   TAU    CM./SEE KK TAU.
V357_  V358   TAU CM./SEE FL TAU.
V359_  V360   TAU CM./SEE KK TAU.
V361   TAU    CM./SEE HZ TAU.
V362   TAU    CM./SEE KK TAU.
V363_  V364   TAU CM./SEE HZ TAU.
V365   TAU    CM./SEE KK TAU.
V366   TAU    CM./SEE FL TAU.
V367_  V369   TAU CM./SEE KK TAU.
V370   TAU    CM./SEE FL TAU.
V371   TAU    VB (DM-1M, 1.5"). CM./SEE FL TAU.
V372   TAU    CM./SEE FL TAU.
V373_  V374   TAU CM./SEE KK TAU.
V375   TAU    CM./SEE SX TAU.
V376_  V378   TAU CM./SEE FL TAU.
V379_  V380   TAU CM./SEE HZ TAU.
V381_  V382   TAU CM./SEE FL TAU.
V383   TAU    CM./SEE KK TAU.
V384   TAU    CM./SEE FL TAU.
V385   TAU    CM./SEE SX TAU.
V386   TAU    TCSN 437. CM./SEE KK TAU.
V387_  V388   TAU CM./SEE KK TAU.
V389   TAU    TCSN 439. CM./SEE KK TAU.
V390   TAU    CM./SEE KK TAU.
V392   TAU    CM./SEE HZ TAU.
V393   TAU    CM./SEE KK TAU.
V394   TAU    CM./SEE SX TAU.
V395_  V397   TAU CM./SEE KK TAU.
V398   TAU    CM./SEE HZ TAU.
V399   TAU    CM./SEE FL TAU.
V400_  V401   TAU CM./SEE KK TAU.
V402_  V403   TAU CM./SEE FL TAU.
V404_  V405   TAU CM./SEE KK TAU.
V410   TAU    HAATC EPOECKE KOEAH ECKA C/
              THERE ARE PERIODICAL LIGHT VARIATIONS WITH P=1.92D,
              A(V)=0.21M, M-M=0.5P  10056!.
V411   TAU    MU=0.13", P=143G. PTBH E KAPK. O-
              HO HAATC KBAEPOECKE KOEAH C
              A=0.3M  EPOAM P0=12.436 MHT  P1=8.237
              MHT (P1/P0=0.6624), KOTOPE HEHEHO MO-
              PTC TPETM EPOOM PL=0.135D (BOMOHO,
              OPTAHM EPOOM CAOO KOMOHEHTA)./
              ERUPTIVE WHITE DWARF. USUALLY THERE ARE QUASI-PERIO-
              DIC VARIATIONS WITH A=0.3M AND PERIODS P0=12.436
              MIN AND P1=8.237 MIN (P1/P0=0.6624) WHICH ARE
              NONLINEARLY MODULATED BY THE THIRD PERIOD PL=0.135D
              (PROBABLY BY THE ORBITAL PERIOD OF A FAINT COMPANION).
V423   TAU    MIN II 15.8.
V425   TAU    CM./SEE SX TAU.
V426_  V429   TAU CM./SEE KK TAU.
V430   TAU    CM./SEE HZ TAU.
V431_  V434   TAU CM./SEE KK TAU.
V435   TAU    CM./SEE HZ TAU.
V436_  V437   TAU CM./SEE SX TAU.
V438   TAU    CM./SEE HZ TAU.
V439_  V440   TAU CM./SEE KK TAU.
V441   TAU    CM./SEE HZ TAU.
V442_  V443   TAU CM./SEE KK TAU.
V444   TAU    CM./SEE HZ TAU.
V445   TAU    CM./SEE KK TAU.
V446   TAU    CM./SEE FL TAU.
V447   TAU    CM./SEE SX TAU.
V448   TAU    CM./SEE FL TAU.
V449   TAU    CM./SEE SX TAU.
V451   TAU    CM./SEE SX TAU.
V452_  V453   TAU CM./SEE HZ TAU.
V454   TAU    CM./SEE SX TAU.
V455_  V460   TAU CM./SEE KK TAU.
V461   TAU    CM./SEE HZ TAU.
V462   TAU    CM./SEE SX TAU.
V463_  V465   TAU CM./SEE KK TAU.
V466   TAU    CM./SEE HZ TAU.
V467_  V469   TAU CM./SEE KK TAU.
V470   TAU    CM./SEE HZ TAU.
V471   TAU    CM./SEE EY TAU; MU ALFA=+0.117", MU DELTA=-0.020".
              EA/D/(RS+WD)+XP. D=0.0625P.
              B MIN I HAAETC OHOE ATMEHE EOO
              KAPKA HO 0.04M V, 0.36M U./THERE OCCURS A
              TOTAL ECLIPSE OF THE WHITE DWARF IN MIN I (A=0.04M V,
              0.36M U).
              P VAR. MIN I=2440612.67083+0.52118321D*E
              (J.D.2440570-970)  6250!; MIN I=2440898.80038+
              +0.52118376D*E (J.D.2440880-41360), MIN I=
              =2441665.46153+0.52118329D*E (J.D.2441660-
              42100)  10058!; OCE/SINCE J.D.2441900-CM.
              TA./SEE TABLE.
              HA KPBO ECKA BHE ATMEH HAAETC MP-
              PEE B HAPABEH MEHEH A BOHOOPA-
              HOE BOMEHE C AMTO OT 0.05M O 0.27M  E-
              POOM, KM K OPTAHOM, A TAKE BCK.
              EPO MPA 191D  10060!  -250D  10061!.
              EPO BPAEH EOO KAPKA O HAEHM
              B PEHTEHOBCKX AX PPULS=554.73S  10062!./
              WAVE-LIKE DISTORSION WITH THE AMPLITUDE FROM 0.05M
              UP TO 0.27M AND WITH THE PERIOD CLOSE TO THE ORBITAL
              ONE IS OBSERVED IN THE LIGHT CURVE OUTSIDE ECLIPSES;
              SOMETIMES THERE ARE ALSO FLARES. THE WAVE IS MIGRA-
              TING ON PHASE IN THE DIRECTION OF PHASE DECREASING
              WITH A MIGRATION PERIOD OF 191D  10060! OR -250D
               10061!. THE PERIOD OF WHITE DWARF ROTATION DERIVED
              THROUGH X-RAY OBSERVATIONS PPULS=554.73S  10062!.
V472   TAU    CM./SEE KK TAU.
V473   TAU    P=2.7800D?
V474   TAU    CM./SEE SX TAU.
V475_  V478   TAU CM./SEE KK TAU.
V479   TAU    VB A (BC 8.90M, 59", 357G); (K-B)2=0.40.
V480   TAU    VB A (B 10.4M, 176", 303G). CM./SEE EY TAU.
V481   TAU    CM./SEE KK TAU.
V483_  V484   TAU CM./SEE EY TAU.
V485   TAU    CM./SEE KK TAU.
V486   TAU    AHA OXA MAX (U)./EPOCH OF MAX (U) IS GIVEN.
              P=/10.61D?  10063!.
V487   TAU    CM./SEE SX TAU. HA KAPTE AA-BBEPX, -
              CPABA./ON THE PHOTOGRAPH WEST IS AT THE TOP AND
              SOUTH TO THE RIGHT.
V488   TAU    CM./SEE FL TAU.
V489_  V490   TAU CM./SEE KK TAU.
V491_  V492   TAU CM./SEE HZ TAU.
V493   TAU    CM./SEE KK TAU.
V494   TAU    CM./SEE SX TAU.
V495_  V496   TAU CM./SEE KK TAU.
V497   TAU    CM./SEE HZ TAU.
V498   TAU    CM./SEE SX TAU.
V499   TAU    CM./SEE KK TAU.
V500   TAU    CM./SEE FL TAU.
V501   TAU    CM./SEE SX TAU.
V502   TAU    CM./SEE FL TAU.
V503   TAU    CM./SEE SX TAU.
V504   TAU    CM./SEE KK TAU.
V506   TAU    CM./SEE SX TAU.
V507_  V516   TAU CM./SEE KK TAU.
V517   TAU    CM./SEE SX TAU.
V518   TAU    VB B (A 14.4M; B 10", 80G). CM./SEE FL TAU.
V519   TAU    CM./SEE SX TAU.
V520   TAU    CM./SEE HZ TAU.
V521   TAU    CM./SEE SX TAU.
V522   TAU    CM./SEE KK TAU.
V523   TAU    CM./SEE SX TAU.
V524   TAU    CM./SEE KK TAU.
V525   TAU    CM./SEE SX TAU.
V526   TAU    CM./SEE KK TAU.
V527   TAU    CM./SEE SX TAU.
V528   TAU    CM./SEE KK TAU.
V529_  V530   TAU CM./SEE SX TAU.
V531_  V533   TAU CM./SEE KK TAU.
V534_  V536   TAU CM./SEE FL TAU.
V537   TAU    CM./SEE KK TAU.
V538   TAU    CM./SEE FL TAU.
V539   TAU    CM./SEE HZ TAU.
V540_  V541   TAU CM./SEE FL TAU.
V542   TAU    CM./SEE SX TAU.
V543_  V544   TAU CM./SEE KK TAU.
V545   TAU    MAX=2444896.678+0.355D*E, M-M=0.42P, A(V)=
              =0.09M  10052!. CM./SEE FL TAU.
V546   TAU    CM./SEE SX TAU.
V547   TAU    CM./SEE KK TAU.
V548   TAU    CM./SEE HZ TAU.
V549   TAU    CM./SEE KK TAU.
V550   TAU    CM./SEE FL TAU.
V551_  V552   TAU CM./SEE KK TAU.
V553   TAU    CM./SEE SX TAU.
V554   TAU    CM./SEE KK TAU.
V555   TAU    CM./SEE SX TAU.
V556   TAU    CM./SEE KK TAU.
V557   TAU    CM./SEE SX TAU.
V558   TAU    CM./SEE KK TAU.
V559_  V560   TAU CM./SEE SX TAU.
V561_  V564   TAU CM./SEE KK TAU.
V565_  V566   TAU CM./SEE SX TAU.
V567_  V568   TAU CM./SEE KK TAU.
V569   TAU    CM./SEE SX TAU.
V570_  V577   TAU CM./SEE KK TAU.
V578   TAU    CM./SEE SX TAU.
V579_  V584   TAU CM./SEE KK TAU.
V585   TAU    CM./SEE IO TAU.
V589   TAU    CM./SEE IO TAU.
V594_  V595   TAU CM./SEE KK TAU.
V596   TAU    CM./SEE HZ TAU.
V597_  V601   TAU CM./SEE KK TAU.
V602   TAU    CM./SEE SX TAU.
V603_  V607   TAU CM./SEE KK TAU.
V608   TAU    CM./SEE SX TAU.
V609   TAU    CM./SEE KK TAU.
V610   TAU    CM./SEE FL TAU.
V611_  V612   TAU CM./SEE KK TAU.
V613   TAU    CM./SEE HZ TAU.
V614   TAU    CM./SEE KK TAU.
V615   TAU    CM./SEE SX TAU.
V617_  V622   TAU CM./SEE KK TAU.
V623   TAU    CM./SEE FL TAU.
V624   TAU    B TAE AHO HAEHE P1(A1=0.01M)./THE VALUE
              OF P1(A1=0.01M) IS GIVEN IN THE TABLE.
              P2=0.017D, A2=0.007M. CM./SEE FL TAU.
V625_  V626   TAU CM./SEE KK TAU.
V627   TAU    CM./SEE FL TAU.
V629_  V630   TAU CM./SEE KK TAU.
V631_  V632   TAU CM./SEE FL TAU.
V633_  V634   TAU CM./SEE SX TAU.
V635   TAU    CM./SEE FL TAU.
V636   TAU    CM./SEE SX TAU.
V637   TAU    CM./SEE KK TAU.
V638   TAU    CM./SEE FL TAU.
V639_  V640   TAU CM./SEE KK TAU.
V641   TAU    MAX=2444896.744+1.22D*E; M-M=0.5P, A(V)=0.03M
               10052!. CM./SEE FL TAU.
V642_  V644   TAU CM./SEE FL TAU.
V645   TAU    CM./SEE HZ TAU.
V646   TAU    CM./SEE FL TAU.
V647   TAU    B TAE AHO HAEHE P1(A1=0.011M)./THE VALUE
              OF P1(A1=0.011M) IS GIVEN IN THE TABLE.
              P2=0.070D, A2=0.006M. CM./SEE FL TAU.
V648_  V649   TAU CM./SEE KK TAU.
V650   TAU    CM./SEE FL TAU.
V651   TAU    CM./SEE KK TAU.
V652   TAU    CM./SEE FL TAU.
V653   TAU    CM./SEE SX TAU.
V654   TAU    CM./SEE HZ TAU.
V655_  V656   TAU CM./SEE KK TAU.
V657   TAU    CM./SEE SX TAU.
V658_  V659   TAU CM./SEE KK TAU.
V660   TAU    MAX=2444896.453+0.23541D*E, M-M=0.5P, A(V)=
              =0.20M  10052!. CM./SEE FL TAU.
V661_  V663   TAU CM./SEE KK TAU.
V664   TAU    CM./SEE FL TAU.
V665   TAU    CM./SEE SX TAU.
V666   TAU    CM./SEE KK TAU.
V667   TAU    CM./SEE FL TAU.
V668_  V671   TAU CM./SEE KK TAU.
V672   TAU    CM./SEE SX TAU.
V673   TAU    CM./SEE HZ TAU.
V674   TAU    CM./SEE KK TAU.
V675   TAU    CM./SEE SX TAU.
V676   TAU    CM./SEE KK TAU.
V677   TAU    CM./SEE FL TAU.
V678   TAU    CM./SEE SX TAU.
V679   TAU    CM./SEE FL TAU.
V680   TAU    CM./SEE SX TAU.
V681_  V683   TAU CM./SEE KK TAU.
V684_  V685   TAU CM./SEE SX TAU.
V686_  V691   TAU CM./SEE KK TAU.
V692   TAU    CM./SEE HZ TAU.
V693_  V694   TAU CM./SEE KK TAU.
V696_  V697   TAU CM./SEE EY TAU.
V698   TAU    T/TYPE INB?
V700   TAU    CM./SEE FL TAU.
V701_  V702   TAU CM./SEE KK TAU.
V703   TAU    CM./SEE FL TAU.
V705_  V707   TAU CM./SEE KK TAU.
V709   TAU    CM./SEE KK TAU.
V710   TAU    VB A (B 16M, 3.5", 180G).
V711   TAU    VB A (B 8.83M, A=8.023", E=0.18, PORB=2101 YR);
              SB2 (PORB=2.83774D  10070!).
              EPO MPA CTOPCOHHO BOH-10.5 ET/
              MIGRATION PERIOD OF THE DISTORTION WAVE IS ABOUT
              10.5 YR  10072!.
              PBEEH PEE MEHEH CMMAPHOO ECKA./
              THE RANGE OF COMBINED LIGHT VARIATION IS GIVEN.
V712_  V717   TAU CM./SEE KK TAU.
V718   TAU    CM./SEE IO TAU.
V725   TAU    SB1 (PORB=110.8D  10076!). PEHTEHOBCKE BCK
              HAATC P POXOEH CAPA  EP-
              ACTPA, OBTOPC C P=PORB. AMTA COOTBET-
              CTBX MEHEH BAHOO ECKA CCTEM
              A(V)=0.03M. EPO BPAEH CAPA PROT VAR
               10077!./X-RAY OUTBURSTS OCCUR PERIODICALLY NEAR
              THE PERIASTRON PASSAGES OF THE PULSAR WITH P=PORB.
              THE AMPLITUDE OF THE CORRESPONDING VARIATIONS OF
              VISUAL BRIGHTNESS OF THE SYSTEM A(V)=0.03M. THE PE-
              RIOD OF PULSAR ROTATION PROT VAR  10077!.
              PROT=104.17S (J.D.2442531), 103.806S (J.D.2442728),
              103.882S (J.D.2443505), 103.8402S (J.D.2443620)
               10074!; 103.647S (J.D.2444521), 103.423S
              (J.D.2445292), 103.3429S (J.D.2445623)  10078!.
V726   TAU    MIN II 11.2.
V727   TAU    CM./SEE KK TAU.
V728   TAU    CM./SEE SX TAU.
V729   TAU    MAX=2439024.46+152.35D*E (J.D.2438680-39415);
              MAX=2440127.78+313.86D*E (J.D.2439415-40510).
              H2O MAEP/MASER.
V732_  V752   TAU CM./SEE KK TAU.
V753   TAU    CM./SEE SX TAU.
V754_  V757   TAU CM./SEE KK TAU.
V758   TAU    CM./SEE SX TAU.
V759_  V760   TAU CM./SEE KK TAU.
V761_  V762   TAU CM./SEE SX TAU.
V763_  V765   TAU CM./SEE KK TAU.
V767_  V772   TAU CM./SEE KK TAU.
V773   TAU    HAATC TAKE KBACHCOAHE MEHE-
              H ECKA C P=3.43D  A(V)=0.13M  10056!./THE-
              RE ARE ALSO QUASISINUSOIDAL LIGHT VARIATIONS WITH
              P=3.43D AND A(V)=0.13M  10056!.
V774   TAU    VB A (B 6.96M, G5IV, 66.8", 315G).
V775   TAU    CM./SEE EY TAU.
V776   TAU    VB A (B 7.5M, 1.4", 333G, 1958; C 8.7M, 77.2", 233G,
              1925); SB 1 (PORB=57.25D). CM./SEE EY TAU.
V777   TAU    VB A (B 8.12M V, 0.0088", 173.2G, 1980.6).
              CM./SEE EY TAU.
V778   TAU    MIN II 17.0. P VAR. MIN I=2438680.546+0.434842D*E
              (J.D.2436528-38841); MIN I=2439765.488+
              +0.434846D*E (J.D.2439559-41031); OCE/SINCE
              J.D.2440129-CM.TA./SEE TABLE.
V780   TAU    VB A (B 15.8M V, 0.3", 310G, 1974); MU=0.364", P=163G.
V781   TAU    MIN II 9.3.
V782_  V784   TAU CM./SEE KK TAU.
V785   TAU    CM./SEE FL TAU.
V787_  V788   TAU CM./SEE KK TAU.
V789_  V790   TAU CM./SEE FL TAU.
V791   TAU    CM./SEE KK TAU.
V792   TAU    POM C V752 TAU. EHTHA C HE?/NEAR V752
              TAU. IDENTICAL TO IT?
              CM./SEE KK TAU.
V793   TAU    CM./SEE FL TAU.
V794   TAU    CM./SEE SX TAU.
V795   TAU    CM./SEE KK TAU.
V796   TAU    CM./SEE FL TAU.
V797   TAU    CM./SEE SX TAU.
V798_  V802   TAU CM./SEE KK TAU.
V804   TAU    CM./SEE KK TAU.
V805   TAU    CM./SEE EY TAU.
V807   TAU    VB A (B=GH TAU, 21.4", 193G).
V808   TAU    PORB=11.93D. CM./SEE EY TAU.
ALFA   TAU    VB A (B 13.5M, M2V, 31", 110G). OKPEHA HPA-
              KPACHO MCCOHHO OOOKO AMETPOM OKOO
              10"./THE STAR IS SURROUNDED BY AN INFRARED EMISSION
              ENVELOPE WITH THE DIAMETER OF ABOUT 10".
              CM./SEE IO TAU.
DZETA  TAU    MIN II 3.05.
TETA** 2      TAU VB A (B 4.85M, 0.02077", 19.6G, 1980.59); SB 1 (PORB=
              =140.728D, E=0.75  10087!).
              B TAE AHO HAEHE P1(A1=0.017M B). P1 VAR.
              OE P1=0.07541D (A1=0.023M B), P2=0.0831D
              (A2=0.013M B)./THE VALUE OF P1(A1=0.017M B) IS
              GIVEN IN THE TABLE. P1 VAR. LATER P1=0.07541D (A1=
              =0.023M B), P2=0.0831D (A2=0.013M B).
              BOMOHO, ATMEHHA C EMEHTAM:/POSSIBLY
              ECLIPSING WITH THE ELEMENTS: MIN=2445358.38+
              +140.734D*E, A=0.02M B.
              CM./SEE EY TAU.
LAMBDA TAU    MIN II 3.54. TPOHA CCTEMA. ATMEHHA CCTEMA
              OPAAETC BOKP TPETEO KOMOHEHTA C P=
              =33.025D  10090!./TRIPLE SYSTEM. THE ECLIPSING SYS-
              TEM ROTATES AROUND THE THIRD COMPONENT WITH P=
              =33.025D  10090!.
              CM./SEE IO TAU.
RO     TAU    CM./SEE EY TAU.
IPSILO TAU    VB A (B 6.5M, 0.020"). CM./SEE EY TAU.
U      TEL    P VAR. O/BEFORE J.D.2421000 MAX=2420992+
              +439.13D*E  0001!; OCE/SINCE J.D.2423000-CM.
              TA./SEE TABLE.
RR     TEL    B 1889-1930 12M-14M PG (COACHO  0625!, HEPA-
              BHE MEHEH; COACHO  0017!, MAX=
              =2411490+384D*E, C HEPABHOCTM). B 1930-
              1944 12.5M-16.5M PG, MAX=2430145+386.73D*E  1649!,
              P TOM OCE 1938 . OTMEEHO BEEHE CPEHE-
              O ECKA  AMT. BCKA OT 14M O 7M B OK-
              TPE 1944. B HTEPBAE J.D.2431500-33000 B
              MAX, 6.5M-7.5M PG; OCE J.D.2433100-OCAEHE
              CPEHEO ECKA. B MAX BCK EPOEC-
              KX KOEAH HE OTMEAOC. B HTEPBAE
              J.D.2441426-44899 5.06M-6.74M J, P=387D  9989!,
              M-M=0.5P; MIN (V)=2442551+374.2D*E (1961-1981),
              EPOECKA ACT DV=0.25M  10029!; 9.8M-
              10.7M B, P=395D (J.D.2443500-45500)  10030!.
              B MAX BCK SP C F5 E MCC. O MEPE OC-
              AEH ECKA PABC OAT MCCOHH
              CEKTP C HM BOOPOA, APEEHHM HM
              METAOB BCOKO CTEEH OHA  P. C
              1970-X . OTMEATC OOC OOEH TIO.
              PAOCTOHK, MK PEHTEHOBCK CTOHK./
              DURING 1889-1930 12M-14M PG (ACCORDING TO  0625!,
              IRREGULAR VARIATIONS; ACCORDING TO  0017!, MAX=
              =2411490+384D*E, WITH IRREGULARITIES). DURING
              1930-1944 12.5M-16.5M PG, MAX=2430145+386.73D*E
               1649!; AFTER 1938 AN INCREASE OF MEAN BRIGHTNESS
              AND OF THE AMPLITUDE WAS NOTED. AN OUTBURST FROM
              14M TO 7M IN OCTOBER, 1944. IN MAX, 6.5M-7.5M PG,
              DURING J.D.2431500-33000; AFTER J.D.2433100 BEGAN
              TO DECLINE ITS MEAN BRIGHTNESS. NEAR THE MAX OF THE
              OUTBURST NO PERIODIC VARIATIONS WAS NOTED. DURING
              J.D.2441426-44899 5.06M-6.74M J, P=387D  9989!,
              M-M=0.5P; MIN (V)=2442551+374.2D*E (1961-1981),
              DV=0.25M FOR PERIODIC CHANGES  10029!; 9.8M-10.7M B,
              P=395D (J.D.2443500-45500)  10030!.
              IN THE MAX OF THE OUTBURST THE SPECTRUM WAS CF5
              WITHOUT EMISSIONS. DURING THE BRIGHTNESS DECLINE A
              RICH EMISSION SPECTRUM WAS FORMED WITH LINES OF
              HYDROGEN, FORBIDDEN LINES OF METALS IN HIGH STAGES
              OF IONIZATION, ETC. SINCE THE 1970-IES TIO ABSORPTION
              BANDS ARE BEING NOTED.
              RADIO SOURCE, SOFT X-RAY SOURCE.
RS     TEL    OPABHE KOEAH/SEMIREGULAR VARIATIONS,
              P=45.8D  8140!. K TOK./IR EXCESS.
RV     TEL    VB (0.6", 294G, 1946). D=0.02P.
SZ     TEL    BOMOHA TOECTBEHHOCT CO BEO/POSSIBLY
              IDENTICAL WITH THE STAR ALFA=18H13M16S, DELTA=-53G39.2',
              1950.0 (RR, 15M-16.5M PG)  10032!.
              CM./SEE TT TEL.
TT_TY  TEL    B OACT APOBOO CKOEH/IN THE REGION
              OF THE GLOBULAR CLUSTER NGC 6584.
UY     TEL    VB.
AG     TEL    NF BEA AP./NF STAR OF A PAIR.
AK     TEL    OEH KPACHA./VERY RED.
AX     TEL     A/H!=-0.7.
BL     TEL    HA MIN II/THE DEPTH OF MIN II-0.1M PG.
              BHE ATMEH HAAETC OPABHA EPE-
              MEHHOCT TA CA (7.09M-7.26M V), HOA
              PECTABEMA EPOOM 65.1D, HO BPEMEHAM
              (1969) HE POCEBAAC./SEMIREGULAR VARIABI-
              LITY OF PULSATIONAL CHARACTER (7.09M-7.26M V) IS OBSER-
              VED OUTSIDE ECLIPSES; SOMETIMES IT MAY BE REPRESEN-
              TED BY P=65.1D, BUT SOMETIMES (1969) IT CANNOT BE
              TRACED.
BO     TEL     A/H!=-0.3.
CK     TEL    VB B (A 15.0M).
DZ     TEL    SF BEA AP./SF STAR OF A PAIR.
FR     TEL    D>=0.23P. MIN II 14.0?
GH     TEL    P-10.342D BOMOEH./IS POSSIBLE.
GM     TEL    VB A.
GY     TEL    MIN II 12.0.
HH     TEL    P VAR CEKA/SLIGHTLY.
HO     TEL    MIN II 8.67.
HR     TEL    BOMOEH T EW C BBOE OM P./EW TYPE
              WITH TWICE LONGER P IS POSSIBLE.
IL     TEL    EMEHT HATC B OTBEPEH./THE ELE-
              MENTS NEED CONFIRMATION.
IQ     TEL    MIN II 12.7.
KK     TEL    B-V:+0.6M: (MIN ECKA/LIGHT).
KN     TEL    VB A (B 16M SF).
LW     TEL    BOMOHO, EHTHA/POSSIBLY IDENTICAL TO NSV
              10695.
MT     TEL    MU ALFA=-0.0127S, MU DELTA=-0.109".
               FE/H!=-1.82. DS=9.9.
MV     TEL    CM./SEE HR TEL.
MZ     TEL    CM./SEE HR TEL.
NN     TEL    MIN II 15.5.
NP     TEL    MIN II 13.3.
NS     TEL    MIN II 9.4.
NV     TEL    MIN II 9.0.
OQ     TEL    SF BEA AP./SF STAR OF A PAIR.
PR     TEL    MIN II 11.35. PAOCTOHK/RADIO SOURCE
              PKS 1925-524.
              KTA HBETA C XAPAKTEPHM BPEMEHEM-5 MH./
              HBETA FLUCTUATES ON-5 MIN TIME SCALE.
PS     TEL    V39 (NGC 6584). BEPOTHO, HE EH CKOEH./
              PROBABLY NON-MEMBER OF THE CLUSTER.
              P=0.1422D /OR 0.1657D BOMOEH/IS POSSIBLE.
PT     TEL    V27 (NGC 6584). HE EH CKOEH./CLUSTER NON-
              MEMBER.
PU     TEL    V24 (NGC 6584). HE EH CKOEH./CLUSTER NON-
              MEMBER.
PV     TEL    SB 2.
PX     TEL    V15 (NGC 6584). HE EH CKOEH./CLUSTER
              NON-MEMBER.
PZ     TEL    SB 2.
R      TRI    P VAR. MAX=2412167+267.3D*E (J.D.2412000-16000);
              MAX=2416972+262.6D*E (J.D.2416000-20000);
              OCE/SINCE J.D.2420000-CM.TA./SEE TABLE.
              MAEP/MASER (H2O).
S      TRI    P VAR. MAX=2418541+248.9D*E (J.D.2418000-31000);
              OCE/SINCE J.D.2431000-CM.TA./SEE TABLE.
T      TRI    P VAR. MAX=2420535+320.6D*E (J.D.2420000-27000);
              OCE/SINCE J.D.2427000-CM.TA./SEE TABLE.
U      TRI    DS=1.3.
V      TRI    MIN II 11.0.
X      TRI    VB A (B 13.3M, 6.7", 55.3G, 1952).
              B MAX OH ECK 8.88./USUAL BRIGHTNESS IN
              MAX 8.88. D=0.013P; MIN II 9.07.
              COACHO  10043!, B MOMEHT J.D.2445594.4550 HA-
              AAC BCKA C BOHM MAKCMMOM PO-
              OTEHOCT 35 MH. (DV=0.33M)./ACCORDING
              TO  10043!, A TWO-PEAKED FLARE-LIKE EVENT OF 35 MIN
              DURATION (DV=0.33M) WAS OBSERVED AT
              J.D.2445594.4550.
              P VAR. MIN=2422722.269+0.9715342D*E
              (J.D.2422700-26600); MIN=2426946.508+
              +0.9715390D*E (J.D.2426600-33400); MIN=
              =2433504.397+0.9715290D*E (J.D.2433400-35500);
              MIN=2435687.422+0.9715352D*E (J.D.2435500-
              39200); MIN=2439375.373+0.9715277D*E
              (J.D.2439200-42500)  7603!; OCE/SINCE
              J.D.2442500-CM.TA./SEE TABLE.
Y      TRI    VAR NO.2 (M33). VB A (B 17.28M B, 26.4" NP).
RS     TRI    VB A (B 11.98M, 6.0", 214G, 1962).
              D=0.016P; MIN II 10.4, MIN II-MIN I=0.56P.
RU     TRI    VB A (B 12M, 21.8", 88G).
              MIN II 11.8:.
RW     TRI    HA MIN I/THE DEPTH OF MIN I 1.12M-2.21M.
              D=0.052P-0.086P, D=0.03P. P VAR?  3434, 9858,
              9859!.
              CHE KTA ECKA BHE ATMEH. EM
              CAEE ECK BHE ATMEH, TEM E MIN. B -
              AX J, K HA AE 0.50P BBEH MIN II HO
              0.16M J  10053!. OCK CEKTP AKKPEOHHOO
              CKA C MCCOHHM HM./STRONG FLUCTUATI-
              ONS OF LIGHT OUTSIDE ECLIPSES. THE LOWER THE BRIGHT-
              NESS OUTSIDE THE ECLIPSE, THE DEEPER THE MIN. IN J, K
              LIGHT MIN II OF 0.16M J DEPTH WAS FOUND AT THE PHASE
              0.50P  10053!. FLAT SPECTRUM OF THE ACCRETION DISC
              WITH EMISSION LINES.
RX     TRI    MAX=2426577+192D*E (J.D.2426500-31800); OCE/
              SINCE J.D.2432800-CM.TA./SEE TABLE.
              COACHO/ACCORDING TO  4029!, P=100D?
RY     TRI    KPACHA./RED.
ST     TRI    MIN II 14.5.
SW     TRI    BOMOEH EKT AKO./BLAZHKO EFFECT IS
              POSSIBLE.
SY     TRI    CM./SEE SW TRI.
TT_TX  TRI    B OACT AAKTK/IN THE REGION OF THE GALA-
              XY M 33.
TZ     TRI    ADS 1697 A (B 6.72M, F6V, SB2, PORB=2.2365D,
              3.9", 71G, 1973); SB2 (P=14.732D).
              BTOPHE KOEAH C XAPAKTEPHM BPEMEHEM
              -100D./SECONDARY VARIATIONS ON-100D TIME SCALE.
              MCC H  K CAII OTMEEHA TOKO  OHO 
              G-BE./H AND K CAII EMISSION WAS NOTED ONLY
              FOR ONE OF THE TWO G-STARS.
R      TRA    SB?
U      TRA    MOMEHT MAX0 (OCHOBHOO TOHA)-CM.TA./FOR
              MOMENTS OF MAX0 (FUNDAMENTAL MODE) SEE TABLE.
              MAX1 (EPB OEPTOH/FIRST OVERTONE)=
              =2443266.05+1.824881D*E.
RR     TRA    MIN II 10.60, DII=0.025P.
RW     TRA    (K-B)2=0.30. DS=1.
TW     TRA    VB.
AS     TRA    MIN II 15.7.
BH     TRA    COACHO  4637!, T L./ACCORDING TO  4637!, L TYPE.
CI     TRA    BOMOHO, /POSSIBLY P<0.3D.
DV     TRA    B TEEHE KA HAATC TP MAX  TP MIN./
              THREE MAX AND THREE MIN ARE OBSERVED DURING A CYCLE.
              MAX1 (FI=0.0P) 13.2M; MAX2 (FI=0.2P) 14.2M; MAX3=
              =(FI=0.6P) 13.5M. MIN1, MIN2, MIN3-16.0M.
EH     TRA    BOMOEH HEOK MIN II./SHALLOW MIN II IS
              POSSIBLE.
EK     TRA    N BEA AP./N STAR OF A PAIR.
              CPEH K ME HOPMAHM MAX-CM.TA.
              CPEH K ME CBEPXMAKCMMAM-442.1D
              (J.D.2435200-39700), 551.5D (J.D.2439700-44050).
              OP B CBEPXMAKCMME DM=0.26M V C P=0.06492D,
              M-M=0.26P/FOR THE MEAN CYCLE BETWEEN NORMAL MA-
              XIMA SEE TABLE. THE MEAN CYCLE BETWEEN SUPERMAXI-
              MA 442.1D (J.D.2435200-39700), 551.5D (J.D.2439700-
              44050). SUPERHUMPS (DM=0.26M V) WITH P=0.06492D,
              M-M=0.26P  9945!.
EL     TRA    MIN II 10.9.
EM     TRA    MIN II 10.4.
EN     TRA    COACHO  7934!, T RV:./ACCORDING TO  7934!,
              RV: TYPE.
EP     TRA    MIN II 9.5.
EQ     TRA    MIN II 9.0.
              P VAR. MIN=2416267.614+2.709220D*E (J.D.2416000-
              29000); OCE/SINCE J.D.2429000-CM.TA./SEE
              TABLE.
ER     TRA    P>220D.
FH     TRA    EMEHT HATC B OTBEPEH./THE ELE-
              MENTS NEED CONFIRMATION.
FK     TRA    CM./SEE FH TRA.
FM     TRA    P>=220D.
GN     TRA    MIN II 12.0.
HP     TRA    OK/DEEP MIN II.
              EMEHT HATC B TOHEH./THE ELEMENTS
              NEED IMPROVEMENT.
HV     TRA    MIN II? 14.8. MIN II-MIN I=0.55P.
IM     TRA    P>=150D. AHA OXA MIN./EPOCH OF MIN IS GIVEN.
IW     TRA    MIN II 14.5:. CM./SEE FH TRA.
KX     TRA    2U 1639-62? P.K.326-10G1.
              CKOPOCT AA O/GAS VELOCITIES UP TO 5000 KM/S
               9958!.
KY     TRA    TRA X-1=A1524-61.
KZ     TRA    4U 1626-67. LX/LOPT-2000. VB B (A 14.9M; B25",
              189G).
              APEHTPECKE APAMETP MCOB/BARYCENT-
              RIC PERIOD PARAMETERS FOR PULSES  4534!: MIN=
              =JED 2443931.2394789; P=7.6776762S, DP/DT=
              =(-4.95+-0.02)*10**-11. DMPULSE=0.02M-0.17M.
              PORB=2491.06S /OR 2492.32S  4558!.
              BCK C DM O 0.4M C HTEPBAAM-20 MH,
              CKOPPEPOBAHHE C PEHTEHOBCKM  4536!./
              FLARES WITH DM UP TO 0.4M WITH INTERVALS-20 MIN
              CORRELATED WITH X-RAY FLARES  4536!.
LP     TRA    VB A (B 11.5M, 25", 123G; C 12.0M, BC 6").
T      TUC    P VAR. MAX=2410138+250.76D*E (J.D.2410000-
              14400); MAX=2414900+248.88D*E (J.D.2414400-
              22000); MAX=2432160+250.00D*E (J.D.2422900-
              35000); OCE/SINCE J.D.2437700-CM.TA./SEE
              TABLE.
U      TUC    CM./SEE UW TUC.
              P VAR. MAX=2421190+258.12D*E (J.D.2412600-
              22000); MAX=2427487+262.83D*E (J.D.2422000-
              28000); MAX=2437808+257.70D*E (J.D.2428000-
              39150); OCE/SINCE J.D.2440900-CM.TA./SEE
              TABLE.
V      TUC    CM./SEE UW TUC.
              HA MIN II/THE DEPTH OF MIN II 0.11M.
W      TUC    (K-B)2=0.09, DS=7:. P VAR?
Z      TUC    B OACT MAOO MAEAHOBA OAKA./IN THE
              REGION OF THE SMALL MAGELLANIC CLOUD.
RR     TUC    CM./SEE Z TUC.
              VB A (B 17M, 6", 90G).
RS_RU  TUC    CM./SEE Z TUC.
RV     TUC    CM./SEE Z TUC. VB.
RW_RZ  TUC    CM./SEE Z TUC.
SS     TUC    CM./SEE Z TUC. HV 1877. PAHEE HEBEPHO OTOECT-
              BAC C HV 1887./EARLIER WAS ERRONEOUSLY IDENTI-
              FIED WITH HV 1887.
ST     TUC    CM./SEE Z TUC.
SU     TUC    CM./SEE Z TUC. HV 1922.
              COACHO  9980!, BOMOHA TAKE TOECTBEHHOCT
              C HV 1920./ACCORDING TO  9980!, ALTERNATIVELY MAY BE
              IDENTICAL TO HV 1920.
SV_SW  TUC    CM./SEE Z TUC.
SX     TUC    CM./SEE Z TUC. VB (B 16M? P).
SY     TUC    CM./SEE Z TUC. MIN II 15.4.
SZ     TUC    CM./SEE Z TUC.
TT     TUC    CM./SEE Z TUC. VB A (B 17M, 8" SP).
TU     TUC    CM./SEE Z TUC.
TV     TUC    CM./SEE Z TUC.
              PACOOEHE EPEMEHHO B 2' K CEBEP OT
              CPD-73G64  9980! CKAET OTOECTBEHE C
              HV 2041./THE VARIABLE'S POSITION IN 2' TO THE NORTH
              OF CPD-73G64  9980! MAKES IT IMPOSSIBLE TO IDENTIFY
              IT WITH HV 2041.
TW_TX  TUC    CM./SEE Z TUC.
TZ     TUC    CM./SEE UW TUC.
              VB A (B 13M SP).
UW     TUC    B OACT MAOO MAEAHOBA OAKA. HE EH
              MMO./IN THE REGION OF THE SMALL MAGELLANIC CLOUD.
              SMC NON-MEMBER.
UX     TUC    CM./SEE UW TUC. B OKPECTHOCTX 47 TUC; BEPOT-
              HO, HE EH CKOEH./IN THE NEIGHBOURHOOD OF 47
              TUC; PROBABLY CLUSTER NON-MEMBER.
              P VAR.  FE/H!=-1.8.
VV_VW  TUC    CM./SEE Z TUC.
VZ     TUC    CM./SEE Z TUC.
XZ     TUC    CM./SEE Z TUC.
YY     TUC    EMEHT HATC B TOHEH; AH TEKE
              EMEHT C OXO   7984!./THE ELEMENTS NEED
              IMPROVEMENT; CURRENT ELEMENTS WITH THE EPOCH FROM
               7984! ARE GIVEN.
              (K-B)2=0.03. DS=8:.
AD     TUC    CM./SEE UW TUC. DS=4.9.
AF     TUC    CM./SEE UW TUC.
AH     TUC    CM./SEE UW TUC. P VAR.
AI     TUC    CM./SEE UW TUC. B OACT APOBOO CKOEH/
              IN THE REGION OF THE GLOBULAR CLUSTER NGC 362. P VAR.
AK     TUC    CM./SEE UW TUC. P VAR.
AL     TUC    CM./SEE UW TUC.
AM     TUC    EMEHT HATC B POBEPKE./THE ELEMENTS
              SHOULD BE CHECKED.
               FE/H!=-1.82. DS=9.9.
AO     TUC    EMEHT HATC B TOHEH./THE ELEMENTS
              NEED IMPROVEMENT.
              DS=5.
AP     TUC    CM./SEE UW TUC.
AQ     TUC    CM./SEE UW TUC. B OACT APOBOO CKOEH/
              IN THE REGION OF THE GLOBULAR CLUSTER 47 TUC.
              MIN II 10.48.
AR     TUC    CM./SEE UW TUC.
AS_AT  TUC    CM./SEE Z TUC.
AU_AV  TUC    CM./SEE UW TUC.
AW_AY  TUC    CM./SEE Z TUC.
BC     TUC    CM./SEE Z TUC.
BD     TUC    CM./SEE UW TUC.
BE     TUC    CM./SEE Z TUC.
BF     TUC    CM./SEE Z TUC.  A/H!=-0.7.
BG     TUC    CM./SEE UW TUC.
BH     TUC    CM./SEE Z TUC. VB A (B 14.28M, 10" N).
BS     TUC    (K-B)2=0.10.
BT_BZ  TUC    CM./SEE Z TUC.
CF     TUC    CM./SEE UW TUC. MK PEHTEHOBCK CTOHK.
              CTOPCOHHA BOHA./SOFT X-RAY SOURCE. DISTORTION
              WAVE. DM=0.057M  10065!. MIN II 7.52.
TETA   TUC    EPO ABHOO KOEAH (A=0.0132M)-CM.TA.
              OTMEAC  PE, HECTAHE ACTOT./FOR
              THE PERIOD OF THE MAIN OSCILLATION (A=0.0132M) SEE
              TABLE. OTHER INSTABLE FREQUENCES WERE ALSO NOTED.
R      UMA    MAEP/MASER (H2O).
S      UMA    S 1.5/6 E. P VAR. MAX=2398325+224.51D*E
              (J.D.2394000-2405000); MAX=2405290+230.20D*E
              (J.D.2405000-10500); MAX=2417530+223.96D*E
              (J.D.2410500-23500); MAX=2426324+228.53D*E
              (J.D.2423500-28800); OCE/SINCE J.D.2428800-
              CM.TA./SEE TABLE.
T      UMA    MAEP/MASER (H2O).
W      UMA    ADS 7494 A (B 12.35M, 6.5", 44G, 1963).
              DI=0.037P; MIN II 8.43, DII=0.028P.
              MK PEHTEHOBCK CTOHK./SOFT X-RAY SOURCE.
              LX/LBOL=1.7*10**-4.
              P VAR. MIN I=2420980.8093+0.333638880D*E
              (J.D.2416000-21000); MIN I=2420980.8093+
              +0.333636993D*E (J.D.2421000-33000)  1760!;
              MIN I=2435918.4169+0.33363832D*E (J.D.2433000-
              41000)  5327!; OCE/SINCE J.D.2441000-CM.TA./
              SEE TABLE.
              OPMA KPBO ECKA, BKA H MHMMOB,
              VAR. OTMEEHA CMEAAC BOHA C DM=0.025M Y
               P-1100D  10067!. B  5788! COOEHO O BCKE
              (DM=1.5M, LAMBDA 3300 A, DLAMBDA=50 A, J.D.2438511.7,
              DT=7 MH). B CCTEME AOBE OTOK, TEMHE
              THA HA OBEPXHOCT KOMOHEHTOB. MCC H 
              K CA II./THE LIGHT CURVE SHAPE, INCLUDING DEPTHS OF
              MINIMA, VAR. A MOVING WAVE WITH DM=0.025M Y AND
              P-1100D  10067! WAS NOTED. A FLARE (DM=1.5M,
              LAMBDA 3300 A, DLAMBDA=50 A, J.D.2438511.7, DT=7 MIN) WAS
              ANNOUNCED  5788!. THE SYSTEM CONTAINS GASEOUS
              STREAMS, DARK SPOTS ON THE SURFACE OF THE COMPONENTS.
              H AND K CAII EMISSION.
Z      UMA    OHO 2 MAX  2 MIN A K./USUALLY 2 MAX AND
              2 MIN DURING A CYCLE.
RV     UMA    P VAR. MAX=2417861.434+0.4680618D*E
              (J.D.2417800-25000); MAX=2425053.675+
              +0.4680654D*E (J.D.2425000-29000)  0188!;
              MAX=2438459.945+0.468062D*E (J.D.2429000-
              40000)  3506!; OCE/SINCE J.D.2440000-CM.TA./
              SEE TABLE.
              EKT AKO/BLAZHKO EFFECT, =92.12D
              (J.D.2436229-38114)  9835!.  VAR.
               FE/H!=-1.04; DS=3.5.
RW     UMA    DI<0.08P; MIN II 10.34, DII=0.10P.
               FE/H!A=-0.1,  FE/H!B=-1.0. P VAR?
              CTOPCOHHA BOHA/DISTORTION WAVE, A=0.11M V.
SS     UMA    B AAKTKE/IN THE GALAXY NGC 5457 (M 101).
SU     UMA    K HOPMAHX MAKCMMOB/THE CYCLE OF NORMAL
              MAXIMA 5D-35D  9782, 3791!.
              HA PAHX HTEPBAAX BPEMEH ECTBT TP PA-
              HX CPEHX HAEH KA CBEPXMAKCMMOB,
              CMEH P PA:/THREE DIFFERENT MEAN VALUES OF
              THE MEAN CYCLE OF SUPERMAXIMA CHANGE EACH OTHER
              BEING ACTIVE AT DIFFERENT TIME INTERVALS: P1=161.5D;
              P2=203.9D; P3=248.1D (<P>=201.7D)  9276!.
              PORB=2.06D/N (N=26, 27, 28) /OR 3.1H.
              OKPEHA CAM AO (AMETPOM 28')  MKX
              PEHTEHOBCKX CTOHKOB./SURROUNDED BY A FAINT
              HALO (28' DIAMETER) OF SOFT X-RAY SOURCES.
SW     UMA    SB. BEPXHEE COEHEHE AKKPEOHHOO CKA/
              SUPERIOR CONJUNCTION OF THE ACCRETION DISC T=
              =2445376.8601+0.0567433D*E  9836!.
SX     UMA    P VAR CHO/STRONGLY. O/BEFORE J.D.2418800
              MAX=2416200.486+0.3071148D*E; MAX=
              =2418800.213+0.3071345D:*E (J.D.2418800-22500)
               0001!; MAX=2422653.5032+0.30711855D*E
              (J.D.2422500-26000)  10083!; MAX=2426400.418+
              +0.3071555D*E (J.D.2426000-29500); MAX=
              =2430000.250+0.3071301D*E (J.D.2429500-34000),
              MAX=2438508.751+0.3071363D*E (J.D.2434000-
              39000); OCE/SINCE J.D.2441500-CM./SEE
              TABLE.
               FE/H!=-1.82, DS=9.9.
SZ     UMA    MU ALFA=-0.4853S, MU DELTA=+0.148".
TU     UMA    P VAR  3506!.  FE/H!=-1.05, DS=7.6.
TW     UMA    D=0.002P; MIN II 12.3:.
TX     UMA    MIN II 7.13. P VAR. MIN I=2416426.801+3.063297D*E
              (J.D.2416000-22000); MIN I=2427926.492+
              +3.063337D*E (J.D.2424200-30000); MIN I=
              =2433440.431+3.063300D*E (J.D.2430000-38000)
               9839!; OCE/SINCE J.D.2438000-CM.TA./SEE
              TABLE.
TY     UMA    P VAR, KBAPATH EH:/NON-LINEAR TERM:
              +6.4D*10**-11*E**2.
              DI=0.05P, DII=0.00P. OPMA KPBO ECKA MEHETC.
              /THE LIGHT CURVE SHAPE VAR.
              12.10<=MIN I<=12.14, 12.06<=MIN II<=12.12.
UX     UMA    OPMA ATMEHHO KPBO ECKA, CPEH POBEH
              ECKA BHE ATMEH, HA MIN VAR. KOHEH
              OT TAHX EMEHTOB OCTAT +-0.002D. HO-
              A HAATC CTPE KOEAH ECKA
              (28.54S<=P<=30.02S)  7304!. MK PEHTEHOBCK
              CTOHK./THE SHAPE OF THE ECLIPSE LIGHT CURVE, THE
              MEAN LEVEL OF LIGHT OUTSIDE ECLIPSES, THE DEPTH OF
              MIN VAR. DEVIATIONS FROM THE TABULATED ELEMENTS MAY
              REACH +-0.002D. RAPID BRIGHTNESS OSCILLATIONS
              (28.54S<=P<=30.02S) ARE SOMETIMES OBSERVED  7304!.
              SOFT X-RAY SOURCE.
UY     UMA    MIN II 12.9.
VV     UMA    MIN II 10.26. P VAR. MIN I=2439245.408+0.6873793D*E
              (J.D.2425600-40200)  9843!; MIN I=2440768.6280+
              +0.687367D*E (J.D.2440200-42700); OCE/SINCE
              J.D.2442700-CM.TA./SEE TABLE.
VX     UMA    MAEP/MASER (H2O).
WX     UMA    MU ALFA=-0.4094S, MU DELTA=+0.955", VB B (A=BD+44G2051,
              DM2, 8.74M V; B 28", 133G; OEE/COMMON MU). CTO-
              HK MKOO PEHTEHOBCKOO EH./SOFT
              X-RAY SOURCE. LX/LV=0.095.
XY     UMA    MU ALFA=-0.0055S, MU DELTA=-0.175".
              P VAR. EMEHT COEPAT KBAPATH EH:/
              NON-LINEAR TERM:+2.77D*10**-11*E**2.
              ECK BHE ATMEH VAR HA 0.16M V. HA MIN I
              0.48M-0.67M, HA MIN II 0.19M. MPPA
              BOHA./THE BRIGHTNESS OUTSIDE ECLIPSES VAR BY
              0.16M V. THE DEPTH OF MIN I IS 0.48M-0.67M, THAT OF
              MIN II IS 0.19M. MIGRATING WAVE.
XZ     UMA    MIN II 10.2. P VAR? MIN=2444986.445+1.2223105D*E
              (J.D.2414990-45000); OCE/SINCE J.D.2445000-
              CM.TA./SEE TABLE.
AA     UMA    MIN II 11.53, MAX II 10.94.
              EMEHT TPET POBEPK./THE ELEMENTS SHOULD
              BE CHECKED.
AC     UMA    VB B (A=BD+65G671, 9.97M V, B-V=+0.50M; B 19",
              114G, 1957).
              KAPTA B  8953! HEBEPHA./THE CHART IN  8953! IS
              WRONG.
AD     UMA    BOMOEH EKT AKO./BLAZHKO EFFECT IS
              POSSIBLE. =35D-40D, DA=0.2M.
AE     UMA    B TAE AH P0 OCHOBHOO TOHA./THE FUNDAMEN-
              TAL MODE P0 IS GIVEN IN THE TABLE.
              P1=0.066527D, PBEAT=0.293616D  9869!.
              MAX 10.86-11.10, MIN 11.46-11.52.
AF     UMA    D=0.05P.
AK     UMA    EMEHT TPET TOHEH./THE ELEMENTS NEED
              IMPROVEMENT.
AN     UMA    AHA OXA MIN EPOECKX (P=PORB) MEHEH
              ECKA C A<=1M B. ECT MIN II. B-V=0.0 B MAKC-
              MME, +0.5 BO BPEM ATMEH; U-B=-1.1. KPO-
              BA OPA B AX B OT -9% O -35%; HE-
              HA OPA 0%-13% C OCTPM MAX B
              MAX ECKA. CTPE MEHEH (A=0.03M; F=0.4-
              0.8 ). CPEH POBEH ECKA  OPMA KPBO
              ECKA VAR. B COCTOH HKO AKTBHOCT (B-
              19M) EPEMEHHOCT ECKA C PORB CEAET, MC-
              COHHE H BH  B TEEHE 10% PORB,
              ECT K TOK. CTOHK MKOO PEHTEHOBCKO-
              O EH, VAR. B CEKTPE MCC H, HEI,
              HEII, NIII, FEII./THE EPOCH OF MIN FOR PERIODIC (P=
              =PORB) LIGHT VARIATIONS WITH A<=1M B IS GIVEN. MIN II
              IS PRESENT. B-V=0.0 IN MAX LIGHT, +0.5 DURING AN
              ECLIPSE; U-B=-1.1. CIRCULAR POLARIZATION IN B LIGHT
              -9% TO -35%; LINEAR POLARIZATION 0%-13% WITH A
              SHARP MAX NEAR MAX LIGHT. RAPID CHANGES (A=0.03M,
              F=0.4-0.8 HZ). THE MEAN LIGHT LEVEL AND THE LIGHT
              CURVE SHAPE VAR. DURING THE LOW STATE (B-19M) THE
              LIGHT VARIABILITY WITH PORB DISAPPEARS, EMISSION LI-
              NES OCCUR ONLY DURING 10% OF PORB, IR EXCESS IS NO-
              TED. SOFT X-RAY SOURCE, VAR. EMISSIONS OF H, HEI,
              HE II, NIII, FEII.
AW     UMA    DI=0.06P:; MIN II 7.08, DII=0.11P. OPMA KPBO
              ECKA MEHETC./THE LIGHT CURVE SHAPE VAR.
              P VAR. MIN I=2442150.4385+0.43873234D*E
              (J.D.2438000-42200); OCE/SINCE J.D.2442200-
              CM.TA./SEE TABLE.
AX     UMA    P VAR. MAX=2435951.354+0.53510D*E (J.D.2435900-
              38200)  4375!; B HTEPBAE/DURING J.D.2445000-
              45900-CM.TA./SEE TABLE.
BE     UMA    D=0.006P.
              BHE ATMEH VAR 14.8M<=B<=16.0M (EKT OTPAE-
              H). HA ATMEH OEE 4.3M (LAMBDA LAMBDA 3330-3700 A),
              1.5M (LAMBDA LAMBDA 5265-6005 A)./OUTSIDE ECLIPSES VAR
              14.8M<=B<=16.0M (REFLECTION EFFECT). THE DEPTH OF EC-
              LIPSES FOR LAMBDA LAMBDA 3330-3700 A IS GREATER THAN 4.3M,THAT
              FOR LAMBDA LAMBDA 5265-6005 A IS 1.5M.
BG     UMA    MIN II 10.93.
              BOMOEH T EW./ALTERNATIVE TYPE EW.
BH     UMA    MIN II 12.3.
BI     UMA    MIN II 15.8.
BK     UMA     FE/H!=-1.29, DS=6.6.
BL     UMA    MIN II 16.2.
BM     UMA    HA MIN II/THE DEPTH OF MIN II 0.80M.
BN     UMA     FE/H!=-1.65, DS=8.9.
BP     UMA    D<=0.04P. EMEHT HATC B OTBEPEH./
              THE ELEMENTS NEED CONFIRMATION.
CE     UMA    B OACT CKOEH AAKTK/IN THE REGION OF THE
              CLUSTER OF GALAXIES ABELL 1213. SN 1966 OMIKRON?
CF     UMA    GROOMBRIDGE 1830 B (A=BD+38G2285, V=6.45M,
              B-V=+0.75M, G8 CKAPK/SUBDWARF, MU ALFA=+0.339S,
              MU DELTA=-5.81"; B 2", 165G).
              BOMOHA BCKA 27 EBPA 1968. OPAHE
              CMMAPHOO ECKA HA 0.6M PG 27 APE 1939
               9881!. BOMOHO, O'EKT HE CECTBET  9882!./
              A POSSIBLE FLARE ON FEBRUARY 27, 1968. A BRIGHTENING
              OF THE COMBINED LIGHT BY 0.6M PG ON APRIL 27, 1939
               9881!. MAYBE THE OBJECT DOES NOT EXIST  9882!.
CH     UMA    PEHTEHOBCK CTOHK/X-RAY SOURCE 1E 1003+67.
              LX/LOPT=0.04.
CM     UMA    P VAR?
CQ     UMA    AHA OXA MAX B AX U  B, COBAAEO C
              MIN B AX V./THE EPOCH OF MAX IN U AND B LIGHT
              COINCIDING WITH THAT OF MIN IN V LIGHT IS GIVEN.
              A(U)=0.06M, A(B)=0.06M.
CR     UMA    AH EMEHT  MAX B OOCE U. B OOCAX B
               V EPOHOCT HE AMETHA./THE ELEMENTS FOR
              MAX IN U LIGHT ARE GIVEN. IN B AND V BANDS NO PERIO-
              DICITY IS APPARENT.
              A(U)=0.03M.
CW     UMA    MU=0.27", P=300G.
DF     UMA    ADS 8242A (B 11.4M, 1.8", 60G, 1960).
              B TAE PBEEH CBEEH O CMMAPHOM
              ECKE./THE DATA FOR COMBINED BRIGHTNESS ARE GIVEN
              IN THE TABLE.
              SB 1, PORB=1.033824D.
              MU ALFA=+0.0131S, MU DELTA=-0.038".
              KPOME CTPX MEHEH (<V>=10.14M, DV=0.05M),
              BOMOH MEEHHE MEHEH./BESIDES RAPID VA-
              RIATIONS (<V>=10.14M, DV=0.05M), LONG TERM VARIA-
              TIONS ARE POSSIBLE.
DG     UMA    BOMOEH EKT AKO./BLAZHKO EFFECT IS
              POSSIBLE.
DK     UMA    MK PEHTEHOBCK CTOHK/SOFT X-RAY SOURCE,
              LG LX/LV=-3.5.  FE/H!=-0.38.
DL     UMA    ATMEH C P=0.42D/ECLIPSES WITH P=0.42D  4706!.
DM     UMA    SB 1 (PORB=7.492D).
              MIN=2444026.97+7.478D*E (1979-1982); 1981-
              1984-CM.TA./SEE TABLE. B 1981-1982 BA MIN
              HA KPBO ECKA./TWO MIN IN THE LIGHT CURVE IN
              1981-1982.
DN     UMA    ADS 8347 ABC (A 7.2M VIS; B 9.0M VIS, 0.121", 142.0G,
              1981.5; C 8.3M VIS, 4.0", 42G, 1980; D=BS 4561,
              A1PCREUSR:, V=7.03M, B-V=+0.01M, 63.0", 114G).
              AH PEE MEHEH CMMAPHOO ECKA TPEX
              KOMOHEHTOB. KAKO KOMOHEHT MEHETC-HEBE-
              CTHO. BEO CPABHEH C KOMOHEHT D./
              THE RANGE OF COMBINED BRIGHTNESS FOR THE THREE COM-
              PONENTS IS GIVEN. IT IS NOT KNOWN WHICH OF THE COMPO-
              NENTS VARIES. THE COMPONENT D WAS USED AS A COM-
              PARISON STAR.
              MIN II 6.73, MIN II-MIN I=0.504P.
EPSILO UMA    SB (P=4.15A).
              HTEPEPOMETPECKA BOHA?/INTERFEROMETRIC
              BINARY? (0.053", 94.5G, 1975.4). B 1976-1983 PA-
              PET BOH P HTEPEPOMETPECKX HA-
              EHX HE ABAOC./IN 1976-1983 ATTEMPTS TO RE-
              SOLVE THE BINARY INTERFEROMETRICALLY WERE NOT SUCCESS-
              FUL.
              B BEMC CKOEH UMA./IN THE UMA MOVING
              CLUSTER; MU ALFA=+0.0131S, MU DELTA=-0.010".
IPSILO UMA    ADS 7534 A (B 11.5M, 11.3", 295G, OEE/COMMON MU).
              MU ALFA=-0.0382S, MU DELTA=-0.156".
              OPMA KPBO ECKA  A MEHTC./THE LIGHT CUR-
              VE SHAPE AND A VAR.
R      UMI    H2O MAEP/MASER.
S      UMI    P VAR. MAX=2422604+321.9D*E (J.D.2413000-
              23000); MAX=2432200+331.5D*E (J.D.2423000-
              32800); MAX=2436080+322.5D*E (J.D.2433000-
              37000); MAX=2439011+326.5D*E (J.D.2437000-
              41500); OCE/SINCE J.D.2441500-CM.TA./SEE
              TABLE.
T      UMI    P VAR. MAX=2428332+315.48D*E (J.D.2416500-
              29500); MAX=2436415+310.05D*E (J.D.2429500-
              37200); MAX=2442389+315.5D*E (J.D.2437200-
              43600); OCE/SINCE J.D.2443600-CM.TA./SEE
              TABLE.
U      UMI    P VAR. MAX=2416975+323.1D*E (J.D.2416500-
              21000); MAX=2428804+331.3D*E (J.D.2421000-
              29780)  0001!; MAX=2429789+320.6D*E (J.D.
              2429780-34600)  0960!; MAX=2434600+331D*E
              (J.D.2434600-36300); MAX=2437853+322.6D*E
              (J.D.2436300-39000); OCE/SINCE J.D.2439000-
              CM.TA./SEE TABLE.
V      UMI    CPEH BEHA VAR/MEAN BRIGHTNESS VAR WITH P2=
              =760D.
W      UMI    MIN II 8.66; D=0.02P. P VAR? B EMEHTAX BOMOEH
              HEHEH EH:/NON-LINEAR TERM IN THE ELEMENTS
              IS POSSIBLE:-7.7D*10**-10*E**2.
X      UMI    P VAR? MAX=2424224+343D*E (J.D.2423800-25100)
               0684!; OCE/SINCE J.D.2438100-CM.TA./SEE
              TABLE.
RR     UMI    SB (PORB=749.4D  9896!).
RT     UMI    MIN II 10.86.
RU     UMI    MIN II 10.20.
RZ     UMI    MIN II 13.5.
ALFA   UMI    VB A (B 8.20M, F3V, 18.3", 218G); SB 1 (PORB=10969D,
              E=0.655  9904!). P VAR. EMEHT COEPAT HEHE-
              H EH:/THERE IS A NON-LINEAR TERM IN THE ELEMENTS:
              +1.9877D*10**-7*E**2.
              B 1982 . AMTA MEHEH ECKA  EBO
              CKOPOCT MEHAC./THE AMPLITUDE OF LIGHT AND
              RADIAL VELOCITY VARIATION DECREASED IN 1982.
              A(V)=0.04M (1984).
GAMMA  UMI    P VAR. MAX=2424301.78+0.14335D*E  10097!; MAX=
              =2427904.468+0.14335D*E  10098!. EMEHT, AH-
              HE B TAE, PECTABT HAEH B 1964-
              1968 ./ELEMENTS GIVEN IN THE TABLE REPRESENT OB-
              SERVATIONS IN 1964-1968. COACHO  9906!, B 1922 .
              VR VAR C P=0.108449D./ACCORDING TO  9906! VR VAR
              IN 1922 WITH P=0.108449D.
EPSILO UMI    VB A (B 12.5M, 76.9", 3G). MIN II 4.21.
S      VEL    MIN II 7.83; D=0.041P. P VAR? PBEEHHE B TA-
              E EMEHT COEPAT KBAPATH EH:/THERE
              IS A NON-LINEAR TERM IN THE ELEMENTS GIVEN IN THE
              TABLE:+4.47D*10**-9*E**2.
W      VEL    P VAR. MAX=2415053+384.3D*E (J.D.2414600-17400);
              MAX=2426080+399.9D*E (J.D.2422400-27300);
              MAX=2429990+388.0D*E (J.D.2427300-30100);
              MAX=2438328+398.7D*E (J.D.2430100-38800);
              OCE/SINCE J.D.2438800-CM.TA./SEE TABLE.
              OH MCC/EMISSION.
Y      VEL    P VAR. MAX=2415900+438.6D*E (J.D.2411500-
              15900); MAX=2419930+447.7D*E (J.D.2415900-
              19930); MAX=2425755+452.8D*E (J.D.2421600-
              27600); MAX=2434150+439.5D*E (J.D.2427600-
              34200); OCE/SINCE J.D.2434200-CM.TA./SEE
              TABLE.
Z      VEL    P VAR. MAX=2415445+435.96D*E (J.D.2415000-
              25100); MAX=2425462+417.99D*E (J.D.2425100-
              29700)  0960!; OCE/SINCE J.D.2429200-CM.TA./
              SEE TABLE.
RR     VEL    MIN II 10.9.
RS     VEL    P VAR. MAX=2410403+421D*E (J.D.2410400-16800)
               9961!; OCE/SINCE J.D.2415450-CM.TA./SEE
              TABLE.
RU     VEL    VB A (B 12M SF). COACHO/ACCORDING TO  0017!,
              MAX=2414390+63D*E.
RW     VEL    P VAR. MAX=2413553+430.4D*E (J.D.2413500-
              18500); MAX=2420610+465.7D*E (J.D.2418500-
              25700); OCE/SINCE J.D.2425700-CM.TA./SEE
              TABLE.
RX     VEL    MIN II 10.5.
RY     VEL     A/H!=-0.3. P VAR. MAX=2440246.67+28.1270D*E
              (J.D.2419000-40250)  5366!; OCE/SINCE
              J.D.2443900-CM.TA./SEE TABLE.
SW     VEL    P VAR. MAX=2434872.95+23.473D*E-3.75D*10**-5*E**2
              (J.D.2412500-35500)  9636!. OCE/SINCE
              J.D.2440700-CM.TA./SEE TABLE.
SX     VEL    KPBA ECKA MEET BOHO MAKCMM. B TA-
              E AHA OXA ABHOO (BTOPOO) MAKCMMA./
              THE LIGHT CURVE HAS DOUBLE MAXIMUM. THE EPOCH OF
              THE PRIMARY (SECOND) MAXIMUM IS GIVEN IN THE TABLE.
TT     VEL    MIN II 10.7.
UW     VEL    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 3033.
YZ     VEL    MIN II 12.8; DII=0.040P; MIN II-MIN I=0.537P.
ZZ     VEL    MIN II 10.0.
AA     VEL    MIN II 10.3.
AC     VEL    MIN II 9.11.
AF     VEL    (K-B)2=0.06. BOMOEH EKT AKO/BLAZHKO
              EFFECT IS POSSIBLE  10110!.
AH     VEL    SB?  10111!. CM./SEE AK VEL.
AI     VEL    MU=0.11", P=76G; (K-B)2=0.23. HA KOEAH EC-
              KA C EPOOM P0, PBEEHHM B TAE, HAKA-
              BATC KOEAH C P1=0.08620868D C OOBH-
              HO AMTO. COACHO  10112! P0 OCTOHEH,
              P1 BOPACTAET./LIGHT OSCILLATIONS WITH THE PERIOD
              P0 GIVEN IN THE TABLE ARE SUPERIMPOSED BY OSCILLA-
              TIONS WITH P1=0.08620868D AND TWICE SMALLER AMPLITU-
              DE. ACCORDING TO  10112! P0 IS CONSTANT, P1 IS INCREA-
              SING.
AK     VEL    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER COLLINDER 173.
AL     VEL    D=0.072P.
AO     VEL    CM./SEE AK VEL.
              MIN II 9.55:. HAAETC BEHE H AC./
              THERE IS APSIDAL LINE MOTION.
              PBEEHHE B TAE EMEHT COEPAT CH-
              COAH EH:+0.058D SIN FI, E FI=
              =2PI(E-5338)/11500, A HAEH E OTCTBATC
              OT OX J.D.2415810.66/THERE IS A SINUSOIDAL TERM
              IN THE ELEMENTS GIVEN IN THE TABLE:+0.058D SIN FI,
              WHERE FI=2PI(E-5338)/11500, AND E VALUES ARE
              COUNTED FROM J.D.2415810.66.
              MIN II=2424270.125+1.5845993D (E-5338)-
              -0.058D SIN FI; MIN II-MIN I=0.792D-0.116D SIN FI.
AP     VEL    P1=2.19984D; P1/P0=0.703. M-M VAR (0.25P<=M-M<=
              <=0.50P)  3710!.
AQ     VEL    D=0.05P. HA MIN II/THE DEPTH OF MIN II 0.05M.
AS     VEL    MIN II 8.4; MIN II-MIN I=0.55P.
AT     VEL    D=0.03P. CM./SEE AK VEL.
AU_AW  VEL    CM./SEE AK VEL.
AX     VEL    B TAE PBEEH EMEHT MEHEH ECKA
              C EPOOM P1 EPBOO OEPTOHA, AMTA KOTOPO-
              O A1 PEBAET AMT HAMEHTAHO MO-
               A0:A1(V)=1.5A0(V).  HAMEHTAHO
              MO P0 MAX HEL=2443878.885+3.673174D*E./THE
              FIRST OVERTONE MODE LIGHT VARIATION ELEMENTS WITH THE
              PERIOD P1 ARE GIVEN IN THE TABLE; THE AMPLITUDE OF
              THE FIRST OVERTONE MODE LIGHT VARIATION A1 EXCEEDS
              THAT OF THE FUNDAMENTAL MODE, A0:A1(V)=1.5A0(V).
              FOR THE FUNDAMENTAL MODE P0 MAX HEL=2443878.885+
              +3.673174D*E.
              P1/P0=0.706; M-M VAR:0.24P<=M-M<=0.50P:.
AY     VEL    MIN II 9.7.
AZ     VEL    MIN II 13.0. CM./SEE AK VEL.
BB     VEL    P<20D. CM./SEE AK VEL.
BC     VEL    MIN II 12.3.
BD     VEL    D=0.04P.
BE     VEL    MIN II 12.5.
BF     VEL    HA MIN II/THE DEPTH OF MIN II 0.04M.
BM     VEL    MIN II 13.0. B OACT PACCEHHOO CKOEH/IN
              THE REGION OF THE OPEN CLUSTER NGC 2547.
              CM.TAKE/SEE ALSO AK VEL.
BO     VEL    MIN II 14.2.
BP     VEL    MIN II 13.7.
BR     VEL    OPMA KPBO ECKA MEHETC./THE SHAPE OF
              THE LIGHT CURVE VARIES.
BT     VEL    MIN II 14.8.
BU     VEL    MIN II 10.96; MIN II-MIN I=0.522P. CM./SEE AK VEL.
BV     VEL    CM./SEE AK VEL.
BW     VEL    MIN II 14.3.
BX     VEL    B OACT PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER TR 10.
BZ     VEL    MIN II 10.4; MIN II-MIN I=0.57P.
CK     VEL    D=0.3D.
CL     VEL    MIN II 13.4.
CR     VEL    D=0.05P.
CS     VEL     A/H!=0.1. BOMOH EH PACCEHHOO CKOE-
              H/POSSIBLE MEMBER OF THE OPEN CLUSTER RUPRECHT 79.
CU     VEL    EPO KOEAH ECKA B CBEPXMAKCMME-
              0.08D, A=0.4M/THE PERIOD OF SUPERHUMPS-0.08D,
              A=0.4M  10115!.
CV     VEL    MIN II 7.17.
CW     VEL    D=0.024P. HA MIN II/THE DEPTH OF MIN II 0.1M PG.
CZ     VEL    MIN II 11.1.
DF     VEL    MIN II 13.4.
DH     VEL    MIN II 13.7.
DK     VEL    VB A (B 12.50M, 22", 315G; C 16M, 10", 60G).
DL     VEL    MIN II 12.1.
DM     VEL    P=123D?
DQ     VEL    MIN II 11.0.
DS     VEL    MIN II 10.8.
DT     VEL    (K-B)2=0.24.
DX     VEL    MIN II 10.3. B PAOHE PACCEHHOO CKOEH/
              IN THE REGION OF THE OPEN CLUSTER COL 213.
EH     VEL    MIN II 13.4.
EL     VEL    CM./SEE AK VEL.
EO     VEL    MIN II 11.90, DII=0.07P. BEHE H AC:/
              APSIDAL MOTION: MIN II-MIN I=3.15D+0.00003D*E.
              MIN II=2441716.75+5.32969D*E.
EP     VEL    B OACT PACCEHHOO CKOEH/IN THE REGION
              OF THE OPEN CLUSTER IC 2395.
ES     VEL    MIN II 12.7.
ET     VEL    MIN II 12.1.
EU     VEL    MIN II 13.8.
EY     VEL    D=0.04P:.
FM     VEL    MIN II 12.9.
FS     VEL    DS=10.
FT     VEL    MIN II 10.5.
FW     VEL    MIN II 10.0.
FX     VEL    MIN II 10.5. CM./SEE BR VEL.
FY     VEL    MIN II 7.03. T/TYPE ELL?  6827!.
FZ     VEL    VB A (B 12.08M, 24.2", 338G).
GG     VEL    VB A (B 11.2M, 6", DALFA=0). P=2.950432D?
GP     VEL    <MIN II>6.90. MIN II-MIN I=0.55P.
              OXA MIN II COBAAET C OXO ATMEH PEHTE-
              HOBCKOO CTOHKA/THE EPOCH OF MIN II COINCIDES
              WITH THE EPOCH OF THE X-RAY SOURCE ECLIPSE (D=0.188P).
              CM./SEE BR VEL.
              BOMOHO HAOEHE OOEPOECKX KOEA-
              H ECKA:/THERE ARE PROBABLY LONG-PERIOD LIGHT
              OSCILLATIONS: MIN=2442681.6+93.3D*E (A-0.02M)
               10051!.
              EPO PEHTEHOBCKX MCOB VAR:/THE PERIOD
              OF X-RAY PULSES VAR: 282.8913S (1975.5)  10125!;
              282.919S (1975.7)  10126!; 282.869S (1976.4),
              282.838S (1976.9)  10127!; 282.80S (1978.9)  10128!;
              282.745S (1979.3), 282.7874S (1980.3), 282.87S (1981.0)
               10129!; 282.93S (1981.9-1982.9); 282.9306S (1983.2)
               10078!.
GV     VEL    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 2660.
HU     VEL    CAP/PULSAR PSR 0833-45.
              B TMAHHOCT/IN THE NEBULA VELA SNR.
              BEA/STAR M  8276!.
              EHE CAPA MEHETC B PAO, OTECKOM
               GAMMA-AAOHE H BOH C P=0.089S./THE PULSED
              RADIATION VARIES IN RADIO, OPTICAL AND GAMMA RAYS
              WITH P=0.089S.
              P VAR  10136-10139!: P=0.089233318274S
              (J.D.2442553-680), P=0.089234713929S (J.D.
              2442700-848), P=0.089244007685S (J.D.2443654-
              676), P=0.089245406487S (J.D.2443719-850)  10137!;
              P=0.089256985348S (J.D.2444795.84)  10138!.
HV     VEL    EH PACCEHHOO CKOEH/A MEMBER OF THE OPEN
              CLUSTER IC 2391.
HW     VEL    P=0.26133D? CM./SEE HV VEL.
HX     VEL    VB A (B 7.1M, 0.3", 313G, 1949); CM./SEE EP VEL.
              MIN II 5.50:.
HY     VEL    VB A (B 5.7M, 76.6"); CM./SEE HV VEL.
              MIN II 4.90.
IL     VEL    A VAR (0.02M<=A<=0.15M). EPO EH/BEAT PERIOD
              10.075D (MIN A=2443175.5+10.075D*E).
IM     VEL    VB A (B 9.73M, 3.3", 179G, 1948). HA BOH BOH
              MEHEH ECKA C EPOOM BPAEH PROT=
              =2.85204D  A=0.03M HAKABATC OC
              C EPOAM/THE DOUBLE WAVE OF LIGHT VARIATIONS
              WITH ROTATION PERIOD PROT=2.85204D AND A=0.03M IS
              SUPERIMPOSED BY OSCILLATIONS WITH THE PERIODS
              P1=0.00812815D (A1=0.0043M), P2=0.00808206D
              (A2=0.0035M), P3=0.00810503D (A3=0.0008M), P4=
              =0.004052519D (A4=0.0009M), P5=0.004064065D
              (A5=0.0004M), P6=0.004041031D (A6=0.0004M),
              P7=0.00815128D (A7=0.0004M)  9208!.
IN     VEL    P=65-70D,
IP     VEL    VB A (B 11.2M V, 2.1", 200G, 1929). P>1.25D.
IQ     VEL    MIN II 12.94; MIN II-MIN I=0.500P.
IS     VEL    A(U) VAR: 0.005M<=A(U)<=0.018M.
IT     VEL    MIN II 7.08. P=23.52D?
GAMMA* *2     VEL VB A (B 4.22M, 41.3", 220G).
              SB2 (PORB=78.5002D  10119!). B OACT HII./IN
              HII REGION.
              T0=2433633.0-OXA HHEO COEHEH KOMO-
              HEHTA O/IS THE EPOCH OF THE CONJUNCTION WHERE THE
              O COMPONENT IS IN FRONT  10119!.
LAMBDA VEL    VB A (B 14.8M, 18.2", 137G).
OMIKRO VEL    CM./SEE HV VEL. P(VR)=2.74D. P=2.76D? SB1? AHA
              OXA MAX ECKA. TECHA BOHA CCTEMA?/THE EPOCH
              OF THE LIGHT MAXIMUM IS GIVEN. CLOSE BINARY SYSTEM?
R      VIR    P VAR. MAX=2381914+145.77D*E (J.D.2338900-
              2402000); MAX=2402321+144.90D*E (J.D.2402000-
              18000); MAX=2418268+145.48D*E (J.D.2418000-
              30000); MAX=2430489+148.32D*E (J.D.2430000-
              34000); MAX=2434193+144.63D*E (J.D.2434000-
              38500); MAX=2438829+147.45D*E (J.D.2438500-
              43000); OCE/SINCE J.D.2443000-CM.TA./SEE
              TABLE.
              MAEP/MASER (SIO).
S      VIR    P VAR. MAX=2399014+374.7D*E (J.D.2398600-
              2405000); MAX=2412970+376.2D*E (J.D.2412000-
              23500, B CPEHEM/ON AVERAGE); MAX=2423502+
              +381.52D*E (J.D.2423500-23000); OCE/SINCE
              J.D.2433000-CM.TA./SEE TABLE.
              MAEP/MASER (H2O, SIO).
T      VIR    MAEP/MASER (OH, H2O, SIO).
V      VIR    P VAR. O/BEFORE J.D.2427000 MAX=2400467+
              +250.17D*E; MAX=2427225+246.54D*E (J.D.2427000-
              31500); OCE/SINCE J.D.2431500-CM.TA./SEE
              TABLE.
W      VIR    AHA OXA MIN./THE EPOCH OF MIN IS GIVEN. P VAR.
              MIN=2404151.168+17.2707D*E (J.D.2403000-23200);
              MIN=2423200.837+17.2634D*E (J.D.2423200-29700);
              OCE/SINCE J.D.2429700-CM.TA./SEE TABLE.
              OPMA KPBO ECKA MEHETC./THE LIGHT CURVE
              SHAPE VAR.
               FE/H!=-1.03.
X      VIR    VB A (B 12M, DK4, 0.6', -50G).
              OPAH 1871  1882 . MOT T CBAH C HE-
              BEPHM OTOECTBEHEM  1651!./THE BRIGHTENINGS
              OF 1871 AND 1882 MAY BE DUE TO MISIDENTIFICATION
               1651!.
Z      VIR    MU ALFA=+0.0098S, MU DELTA=-0.120".
              P VAR. MAX=2409683+309.19D*E (J.D.2408000-
              18500); OCE/SINCE J.D.2418500-CM.TA./SEE
              TABLE.
RS     VIR    MAEP/MASER (OH, H2O, SIO).
              P VAR. MAX=2412592+351.29D*E (J.D.2412000-
              31000); OCE/SINCE J.D.2431000-CM.TA./SEE
              TABLE.
RT     VIR    MAEP/MASER (OH, H2O, SIO).
              COACHO  10145!, HAEH 1970-1977 POTBO-
              PEAT KAAHHOM B TAE HAEH P./ACCORDING
              TO  10145!, OBSERVATIONS OF 1970-1977 ARE NOT IN AG-
              REEMENT WITH THE P VALUE IN THE TABLE.
RU     VIR    P VAR? MAX=2425120+435.9D*E (J.D.2414000-
              31500); OCE/SINCE J.D.2431500-CM.TA./SEE
              TABLE.
RV     VIR    P VAR. MAX=2412272+268.39D*E (J.D.2412000-
              31500); OCE/SINCE J.D.2431500-CM.TA./SEE
              TABLE.
RX     VIR    VB (B 13.0M VIS, 1.1", 107G, 1939).
              O OTOEKTPECKM HAEHM/ACCORDING TO
              PHOTOELECTRIC OBSERVATIONS  6450, 8837!, 8.72M-8.81M V.
              CONST?  6450!.
SS     VIR    P VAR. MAX=2415910+352.75D*E (J.D.2415900-
              21500); MAX=2421913+361.7D*E (J.D.2421500-
              26500); MAX=2428359+350.12D*E (J.D.2426500-
              40000); OCE/SINCE J.D.2440000-CM.TA./SEE
              TABLE.
ST     VIR    P VAR. MAX=2425005533+0.4108494D*E (J.D.2422000-
              29100)  10146!; MAX=2436702.513+0.4108168D*E
              (J.D.2433000-39000)  3415!; OCE/SINCE
              J.D.2439000-CM.TA./SEE TABLE. EKT A-
              KO?/BLAZHKO EFFECT?
              DS=0.8.
SU     VIR    P VAR. MAX=2415040+213.7D*E (J.D.2415000-19500);
              MAX=2419926+210.96D*E (J.D.2415000-31500);
              MAX=2437378+210.2D*E (J.D.2431500-38500); OC-
              E/SINCE J.D.2438500-CM.TA./SEE TABLE.
SV     VIR    P VAR? AH CPEHE EMEHT./THE MEAN ELEMENTS
              ARE GIVEN.
              MAEP/MASER (H2O).
SZ     VIR    BOMOHO, EW C OEH MAO A./POSSIBLY EW
              WITH A VERY SMALL A.
TV     VIR    VB A (B P).
TW     VIR    PORB=0.182666D  9430!.
              B AX H EPEMEHHOCT COAHOO XAPAK-
              TEPA:/VARIABILITY OF ELLIPSOIDAL CHARACTER IN H
              LIGHT: P=PORB/2, A(H)=0.13M.
              PEHTEHOBCK CTOHK./X-RAY SOURCE.
TX     VIR    VB A (B 15M, 0.3' P).
TY     VIR     FE/H!=-1.7.
TZ     VIR    P2=6900D HAKABAETC?/IS SUPERIMPOSED?
UU     VIR     FE/H!=-0.3. DS=0.7.
UW     VIR    D=0.011P.
              P VAR. MIN=2419942.513+1.8106818D*E (J.D.
              2415000-34500); OCE/SINCE J.D.2441000-CM.
              TA./SEE TABLE.
UY     VIR    D=0.014P; MIN II 8.1.
VV     VIR    MIN II 12.2:.
VW     VIR    SN 1895 (NGC 4424).
XX     VIR     FE/H!=-1.5. DS=9:.
YZ     VIR     A/H!=-0.9.
AD     VIR    P VAR. MAX=2425259.259+0.5522109D*E
              (J.D.2419000-31000); OCE/SINCE J.D.2431000-
              CM.TA./SEE TABLE.
AF     VIR    P VAR. MAX=2429051.697+0.4838214D*E
              (J.D.2419500-36000); MAX=2436718.3758+
              +0.4838386D*E (J.D.2436000-37500)  10159!;
              OCE/SINCE J.D.2440000-CM.TA./SEE TABLE. DM VAR.
AG     VIR    HA MIN II O/THE DEPTH OF MIN II UP TO 0.44M.
              OPMA KPBO ECKA  A MEHTC./THE LIGHT CUR-
              VE SHAPE AND A VAR.
              DI=0.03P:, DII=0.66P. MIN II-MIN I=0.512P.
              P VAR. MIN=2434487.4297+0.6426489D*E (J.D.
              2424500-34500); OCE/SINCE J.D.2434500-CM.
              TA./SEE TABLE.
AH     VIR    MU ALFA=+0.0015S, MU DELTA=-0.111"
              ADS 8472 A (B 13.2M, 1.3", 17G). AH CMMAPH
              ECK./THE COMBINED BRIGHTNESS IS GIVEN,
              DI=0.07P. HA/THE DEPTH OF MIN II 0.53M, DII=
              =0.00P.
              OPMA KPBO ECKA MEHETC./THE LIGHT CURVE
              SHAPE VAR.
              P VAR. MIN=2434841.3963+0.40751843D*E
              (J.D.2425000-35000)  5222!; MIN=2435573.710+
              +0.40752192D*E (J.D.2435000-41400); MIN=
              =2441411.460+0.40753186D*E (J.D.2441400-44000);
              OCE/SINCE J.D.2444000-CM.TA./SEE TABLE.
AK     VIR    VB B (A=BD-17G3996; B 44", 286G).
AL     VIR    P VAR?  A/H!=-0.7.
AN     VIR    P2-1000D HAKABAETC/IS SUPERIMPOSED.
AO     VIR    VB A (B 11.4M VIS, 6.9", 321G, 1956, OA/COMMON
              VR). DM, BOMOHO, CKAEHA CTHKOM./DM IS
              POSSIBLY IN ERROR BECAUSE OF THE COMPANION.
              P VAR. MAX=2413949+256.88D*E (J.D.2412900-
              21000); OCE/SINCE J.D.2421000-CM.TA./SEE
              TABLE.
AS     VIR    P VAR. B TAE-CPEHE EMEHT OCE
              J.D.2425600./THE TABLE GIVES THE MEAN ELEMENTS
              VALID AFTER J.D.2425600. EKT AKO?/BLAZHKO
              EFFECT?  3506!.
              (K-B)2=0.08.
AT     VIR    P VAR. MAX=2426831.367+0.5258053D*E (J.D.
              2420500-35000)  0188!; OCE/SINCE J.D.2435000-
              CM.TA./SEE TABLE.
              (K-B)2=0.00, DS=6.0.
AU     VIR     FE/H!=-1.84, DS=10.1.
AV     VIR    DS=5.5.
AW     VIR    MIN II 11.67.
AX     VIR    MIN II 10.24.
AY     VIR    MAEP/MASER (H2O).
AZ     VIR    MIN II 11.37.
BB     VIR    EKT AKO?/BLAZHKO EFFECT?
BC     VIR    P VAR. MAX=2419922.289+0.56451468D*E
              (J.D.2419900-30100); B TAE AH TEKE E-
              MEHT./THE TABLE GIVES CURRENT ELEMENTS.
BD     VIR    P VAR. MIN=2424971.720+2.548410D*E
              (J.D.2424900-32000); OCE/SINCE J.D.2432000-
              CM.TA./SEE TABLE.
BF     VIR    MIN II 10.72. ATMEH OHE./TOTAL ECLIPSES.
              P VAR. MIN=2416595.67+0.64057D:*E (J.D.2414000-
              19000); MIN=2440331.809+0.64057631D*E
              (J.D.2426000-41000); OCE/SINCE J.D.2441000-
              CM.TA./SEE TABLE.
BH     VIR    MIN II 10.24. CTOPCOHHA BOHA?/DISTORTION WAVE?
              (DV=0.04M).
BN     VIR    P VAR. MAX=2419865.422+0.39127585D*E
              (J.D.2419800-28300); OCE/SINCE J.D.2432600-
              CM.TA./SEE TABLE.
BO     VIR    P VAR. MAX=2419513.388+0.52005916D*E
              (J.D.2419500-33000); OCE/SINCE J.D.2433000-
              CM.TA./SEE TABLE.
BQ     VIR    P VAR?
BS     VIR     FE/H!=-1.84. DS=10.1.
BV     VIR    P VAR. MAX=2426070.488+0.4965803D*E
              (J.D.2419900-28500); OCE/SINCE J.D.2436600-
              CM.TA./SEE TABLE.
BW     VIR    P VAR. MAX=2420247.403+0.4706660D*E
              (J.D.2420200-26800); OCE/SINCE J.D.2426800-
              CM.TA./SEE TABLE.
CG     VIR    MIN II 10.9.
CK     VIR     FE/H!=-2.0.
CM     VIR    D=0.05P. P VAR. MIN=2425411.330+3.40167D*E
              (J.D.2423900-28400)  0001!; B HTEPBAE/DURING
              J.D.2432200-34200-CM.TA./SEE TABLE.
CS     VIR    AHA OXA MAX B AX B./THE EPOCH OF MAX IN B
              LIGHT IS GIVEN.
              SB (PORB=1618D).
              K TOK/IR EXCESS (4.8 MU M).
CU     VIR    ADS 9152 A (B 11.9M, G1V, 60", 212G).
CW     VIR    AHA OXA MIN./THE EPOCH OF MIN IS GIVEN.
CX     VIR    HA MIN II/THE DEPTH OF MIN II 0.30M.
DK     VIR    COACHO/ACCORDING TO  10189!, P1=0.1162D, P2=
              =0.1086D. (K-B)2=0.20.
DL     VIR    SB (PORB=2286D). B CEKTPE POBETC A-KOMO-
              HEHT ATMEHHO CCTEM  BEA G8III, BOKP
              KOTOPO OPAAETC ATMEHHA CCTEMA./THE
              SPECTRUM SHOWS THE A-COMPONENT OF THE ECLIPSING
              SYSTEM AND THE G8III STAR AROUND WHICH THE ECLIPSING
              SYSTEM IS ORBITING.
DM     VIR    MIN II 9.49. DII=DI.
DN     VIR    P>=100D.
DT     VIR    MU ALFA=-0.044S, MU DELTA=-0.02". SB? EPO
BPAEH/ROTA-
              TION PERIOD 1.535D  10014!, A=0.05M V.
DV     VIR    EKT AKO?/BLAZHKO EFFECT?
EF     VIR    COACHO/ACCORDING TO  4784!, CONST?, 16.1M PG.
EP     VIR    K TOK/IR EXCESS (4.8 MU M).
EQ     VIR    SB;  FE/H!=-0.08; MU ALFA=-0.018S, MU DELTA=-0.09".
              MIN=2441129.585+3.914169D*E+0.0001803345D*E**2,
              A=0.10M V, M-M=0.40P.
              MK PEHTEHOBCK CTOHK/SOFT X-RAY SOURCE,
              LG FX/FV=-2.07.
EW_EY  VIR    P>=100D.
FF     VIR    AH P MEHEH MAHTHOO O./THE P VALUE FOR
              MAGNETIC FIELD VARIATIONS IS GIVEN.
FG     VIR    ADS 8471 A (B 13.51M, 25", 352G, 1909;
              C 11.85M, 74", 195G, 1909).
FI     VIR    MU ALFA=+0.043S, MU DELTA=-1.22".
FL     VIR    VB AB (A=0.76", P=16A). OA KOMOHEHTA BCX-
              BAT? AH PEE MEHEH CMMAPHOO
              ECKA./BOTH COMPONENTS SHOW FLARES? THE RANGE
              OF COMBINED BRIGHTNESS IS GIVEN.
              MU ALFA=-0.118S, MU DELTA=+0.26".
FM     VIR    SB2, PORB=38.324D.
FN     VIR    MU ALFA=-0.064S, MU DELTA=+0.28". SB? PEHTEHOBCK CTO-
              HK/X-RAY SOURCE, LX/LBOL=-3.55.
FO     VIR    MIN II 6.67.
FQ     VIR    OK/DEEP MIN II.
GG     VIR    MTEPOHOCT/MULTIPERIODICITY,
              0.023D<=P<=0.083D, A<=0.02M.
GH     VIR    P VAR.
GK     VIR    BTOPH KOMOHEHT-KPACH KAPK/THE SECON-
              DARY IS A RED DWARF (M0-M6).
GL     VIR    MU ALFA=-0.087S; MU DELTA=+0.23".
GM     VIR    P=1.6D/N.
GQ     VIR    MU ALFA=-0.045S, MU DELTA=-0.44".
GR     VIR    HA MIN II/THE DEPTH OF MIN II 0.41M.
GU     VIR    P VAR. MAX=2439236.36+0.466562D*E
              (J.D.2438100-39300); B HTEPBAE/DURING
              J.D.2441300-42600-CM.TA./SEE TABLE.
ALFA   VIR    B TAE AH OXA MIN COAHO EPE-
              MEHHOCT  PORB./THE TABLE GIVES THE EPOCH OF
              MIN FOR THE ELLIPSOIDAL VARIABILITY AND PORB.
              HA MIN II O 0.08M./THE DEPTH OF MIN II UP TO
              0.08M. SB 2. E=0.205+-0.004. BPAEHE H AC:
              /APSIDAL MOTION: =108A+-5A.
              CA/PULSATIONS: P VAR, P=0.17378587D
              (1908-1956); OCE/SINCE 1956 MAX=2445405.63+
              +0.17378680D*E  10181!. A VAR.
              3 CTHKA O HAEHM HHX OKPT/
              3 COMPANIONS ACCORDING TO LUNAR OCCULTATION OBSER-
              VATIONS: 3.1M, 0.0025"; 4.5M, 0.05"; 7.5M, 0.5".
              MK PEHTEHOBCK CTOHK/SOFT X-RAY SOURCE,
              LX/LBOL=2.9*10**-8.
PSI    VIR    BOHA? (OKPT HO)./BINARY? (LUNAR OCCUL-
              TATIONS).
R      VOL    P VAR. MAX=2415238+441D*E (J.D.2394100-
              2418800)  10143!; OCE/SINCE J.D.2422700-CM.
              TA./SEE TABLE.
S      VOL    P VAR. MAX=2415042+397.6D*E (J.D.2415000-24200),
              MAX=2428880+392.1D*E (J.D.2423000-28900),
              MAX=2434113+401.7D*E (J.D.2428900-34900),
              MAX=2434910+387.2D*E (J.D.2434900-39200);
              OCE/SINCE J.D.2439200-CM.TA./SEE TABLE.
T      VOL    P VAR. MAX=2413135+189.8D*E (J.D.2413100-14600);
              MAX=2416870+171.8D*E (J.D.2414600-16900);
              MAX=2416870+176.8D*E (J.D.2416800-24400);
              MAX=2424460+170.8D*E (J.D.2424400-27200);
              MAX=2429925+182.3D*E (J.D.2427200-30000);
              OCE/SINCE J.D.2440000-CM.TA./SEE TABLE.
RX     VOL    P<20D?
ST     VOL    SP KOMOHEHT OEH TECHO AP./SP COMPONENT OF
              A VERY CLOSE PAIR.
SV     VOL    OPMA KPBO ECKA MEHETC./THE SHAPE OF THE
              LIGHT CURVE VARIES.
TX     VOL    MIN II 10.5. P VAR. MIN I=2416789.869+5.38845D*E
              (J.D.2415100-26000), MIN I=2431150.345+
              +5.3887D*E (J.D.2426000-31400), MIN I=
              =2433542.609+5.388D*E (J.D.2431400-33600)
               0001!; OCE/SINCE J.D.2433600-CM.TA./SEE
              TABLE.
R      VUL    P VAR. MAX=2400169+138.3D*E (J.D.2400100-02700),
              MAX=2402779+136.76D*E (J.D.2402700-19800),
              MAX=2419880+137.45D*E (J.D.2419800-24400),
              MAX=2424413+136.76D*E (J.D.2424400-28500
               0960!; MAX=2429331+135.9D*E (J.D.2428500-32000)
               0001!; OCE/SINCE J.D.2432000-CM.TA./SEE
              TABLE.
S      VUL    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER C 1947+272  10123!.
              P VAR. MAX=2401772+67.37D*E (J.D.2401760-6400),
              MAX=2408180+67.70D*E (J.D.2408170-14950),
              MAX=2415285+68.26D*E (J.D.2415300-22800),
              MAX=2423468+67.72D*E (J.D.2423450-27200),
              MAX=2428227+68.18D*E (J.D.2428220-31300)
               0761!; MAX=2432775+67.51D*E (J.D.2431300-
              34500)  10148!; MAX=2437150+68.66D*E
              (J.D.2436800-39600), MAX=2441507+67.344D*E
              (J.D.2439600-43000)  10124!; OCE/SINCE J.D.
              2443000-CM.TA./SEE TABLE.
               A/H!=0.1.
T      VUL    P VAR. MAX=2419372.151+4.435589D*E (J.D.2409880-
              34000); OCE/SINCE J.D.2434000-CM.TA./SEE
              TABLE.
V      VUL    MIN II 8.65. P VAR. MIN I=2414912.9+74.96D*E
              (J.D.2414900-20840),  MIN I=2420909.8+75.686D*E
              (J.D.2420900-24810), MIN I=2425072.9+76.344D*E
              (J.D.2425050-30000), MIN I=2430023.5+75.957D*E
              (J.D.2430000-32500)  10149!.
              CCEOBAHE MEHEH P  CMEH MIN II HA MIN I
              CM.TAKE B  0767, 10150!./STUDY OF PERIOD VARIATION
              AND CHANGES OF MIN II BY MIN I SEE ALSO IN  0767,
              10150!.
W      VUL    B PAOHE PACCEHHX CKOEH/IN THE REGION OF
              THE OPEN CLUSTERS NGC 6882, NGC 6885.
X      VUL    P VAR. MAX=2420636.337+6.319301D*E (J.D.2417000-
              34000)  0768!; OCE/SINCE J.D.2435000-CM.TA./
              SEE TABLE.
Z      VUL    VB A (B 12.0M, 13", 359G). MIN II 7.58. P VAR. MIN I=
              =2425456.117+2.454926D*E (J.D.2413200-37000)
               0063!; OCE/SINCE J.D.2437000-CM.TA./SEE
              TABLE.
RS     VUL    MIN II 6.86; MIN II-MIN I=0.508P.
RU     VUL    A VAR. P VAR. MAX=2416266+155.95D*E
              (J.D.2415000-36000), MAX=2436779+150.7D*E
              (J.D.2436000-38800), MAX=2438855+153.4D*E
              (J.D.2438800-41620), MAX=2441193+138.5D*E
              (J.D.2441620-42600); OCE/SINCE J.D.2442600-
              CM.TA./SEE TABLE.
RX     VUL    P VAR. MAX=2420301+438D*E (J.D.2418900-22500)
               4018!; OCE/SINCE J.D.2424700-CM.TA./SEE
              TABLE.
RZ     VUL    HA MEEHHE KOEAH CPEHEO ECKA C P=
              =1410D  A=2M HAKABATC KTA C
              KOM OT 40 O 100D  A O 1M./SLOW VARIATIONS
              OF MEAN BRIGHTNESS WITH P=1410D AND A=2M ARE SU-
              PERIMPOSED BY FLUCTUATIONS WITH THE CYCLE 40-100D
              AND A UP TO 1M.
SU     VUL    CM./SEE W VUL.
SV     VUL     FE/H!=0.23. P VAR. PBEEHHE B TAE EMEH-
              T COEPAT KBAPATH EH:/THERE IS A NONLI-
              NEAR TERM IN THE ELEMENTS GIVEN IN THE TABLE:
              -0.0001814D*E**2.
SX     VUL    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6940.
UU     VUL    KOOPHAT OOH?/THE CO-ORDINATES ARE WRONG?
               10156!.
VV     VUL    MIN II 12.1; D=0.026P. P VAR. MIN I=2416670.527+
              +3.411224D*E (J.D.2416600-27500)  0134!; OCE/
              SINCE J.D.2426000-CM.TA./SEE TABLE.
VW     VUL    PORB=0.0731D  10160!.
VY     VUL    MIN II 14.4:.
WW     VUL    OCAEH ECKA POCXOT C KOM 404D./THE-
              RE IS QUASI-PERIODICITY IN LIGHT MINIMA WITH THE CYCLE
              404D.
XZ     VUL    MIN II 11.4. P VAR. MIN I =2426477.525+3.0895116D*E
              (J.D.2416900-36000)  4427!; OCE/SINCE
              J.D.2436000-CM.TA./SEE TABLE.
AB     VUL    HA MIN II/THE DEPTH OF MIN II 0.02M.
AD     VUL    MIN II 0.010P.
AF     VUL    MIN=2436545.23+0.954D*E (J.D.2436200-900)  3148!.
AR     VUL    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER STOCK 1.
AT     VUL    MIN II 9.3; D=0.02P.
AW     VUL    MIN II 10.9; D=0.020P.
AX     VUL    D=0.018P.
AY     VUL    D=0.020P. P VAR. MIN HEL=2436128.388+2.4124239D*E
              (J.D.2418500-40700); OCE/SINCE J.D.2440700-
              CM.TA./SEE TABLE.
AZ     VUL    MIN II 11.9.
BB     VUL    B PAOHE PACCEHHOO CKOEH/IN THE REGION OF
              THE OPEN CLUSTER NGC 6940.
BE     VUL    VB A (BC 11.92M, 50", 320G). MIN II 9.90. P VAR.
              MIN I=2426144.490+1.55205D*E
              (J.D.2426140-28880), MIN I=2430698.203+
              +1.5520442D*E (J.D.2430690-34660), MIN I=
              =2435340.373+1.552052D*E (J.D.2435340-40070);
              OCE/SINCE J.D.2440100-CM.TA./SEE TABLE.
BF     VUL    EMEHT, PBEEHHE B TAE, XOPOO PE-
              CTABT TOKO PKE MAKCMM. OEE CAE
              MAKCMM PECTABTC EMEHTAM: MAX=
              =2427731+95.4D*E./ELEMENTS GIVEN IN THE TABLE
              REPRESENT WELL ONLY THE BRIGHT MAXIMA. THE FAINTER
              MAXIMA ARE REPRESENTED BY THE ELEMENTS: MAX=
              =2427731+95.4D*E.
BI     VUL    MIN II 14.86. P VAR? MIN I=2424759.70+0.251828D*E
               0193!; OCE/SINCE J.D.2444750-CM.TA./SEE
              TABLE.
BN     VUL    DS=7. P VAR. MAX=2414815.759+0.5941295D*E
              (J.D.2414000-30000)  0388!; MAX=2434244.333+
              +0.59412538D*E (J.D.2430000-36000)  0616!;
              MAX=2438265.386+0.59412763D*E (J.D.2436000-
              41000)  9009!; OCE/SINCE J.D.2441000-CM.TA.
              /SEE TABLE.
BO     VUL    MIN II 10.6. P VAR. MIN I=2429984.332+1.9459123D*E
              (J.D.2415000-30000)  0007!; MIN I=2432379.766+
              +1.9459206D*E (J.D.2427000-35000), OCE/SINCE
              J.D.2435300-CM.TA./SEE TABLE.
BP     VUL    MIN II 10.5.
BS     VUL    MIN II 11.10.
BT     VUL    D=0.03P; MIN II 12.3.
BU     VUL    P VAR. MIN=2431006.204+0.5689904D*E
              (J.D.2426500-31100)  0001!; OCE/SINCE
              J.D.2433500-CM.TA./SEE TABLE.
BV     VUL    S 6.5/6-.
BW     VUL    P VAR. MAX=2424000.171+0.20102229D*E
              (J.D.2424000-26500), MAX=2426500.079+
              +0.20102933D*E (J.D.2426500-31500), MAX=
              =2432000.054+0.20103513D*E (J.D.2431500-41000);
              OCE/SINCE J.D.2441000-CM.TA./SEE TABLE.
CD     VUL    MIN II 11.9.
CK     VUL    MAX 2331186:. CBAHA C TMAHHOCTM./CONNECTED
              WITH NEBULAE.
              T/TYPE NR?
CS     VUL    MIN II 13.6.
DR     VUL    MIN II 9.19; DII=0.132P. HAAETC BPAEHE -
              H AC C EPOOM 37.8 ET. PBEEHHE B TA-
              E EMEHT COEPAT OOHTEHE EH:/
              THERE IS APSIDAL MOTION WITH THE PERIOD 37.8 YEARS.
              ELEMENTS GIVEN IN THE TABLE CONTAIN SUPPLEMENTARY
              TERMS:-0.07165D*SIN (0.05863G*E)-0.00269D*
              *SIN (0.11726G*E).
              MIN II=2440301.7934+2.2508645D*E+0.07165D*
              *SIN (0.05863G*E)-0.00269D SIN (0.11726G*E).
              P VAR?  10185!. HA MHMMOB MEHETC./THE
              DEPTH OF MINIMA VARIES.
DY     VUL    VB A (B 13.0M V, 14", 300G).
EH     VUL    P VAR. MAX=2429609+185D*E (J.D.2429600-30600);
              OCE/SINCE J.D.2430800-CM.TA./SEE TABLE.
EP     VUL    S 6.5/5.
EQ     VUL    MIN II 12.5; MIN II-MIN I=0.31P; DII=0.050P, DII=
              =0.010P.
ER     VUL    P VAR. MIN I=2440182.2593+0.69809510D*E
              (J.D.2433100-40200)  8592!; OCE/SINCE J.D.
              2440100-CM.TA./SEE TABLE.
              7.35M<=MIN II<=7.44M. OPMA KPBO ECKA  -
              H MHMMOB MEHTC./THE SHAPE OF THE LIGHT
              CURVE AND DEPTHS OF MINIMA VARY.
ES     VUL    VB A (B 10.1M, 1.6", 126G).
ET     VUL     A/H!=-0.4. P VAR. MAX=2425110.63+54.33D*E
              (J.D.2422900-26600), MAX=2432875.80+54.33132D*E
              (J.D.2432700-35430), MAX=2438656.99+53.81D*E
              (J.D.2436050-39035), MAX=2439253.55+54.24D*E
              (J.D.2439035-40990)  10168!; OCE/SINCE
              J.D.2441900-CM.TA./SEE TABLE.
EU     VUL    MIN II 13.3.
EV     VUL    MIN II 11.9. P VAR. MIN I=2428750.459+2.822084D*E
              (J.D.2428400-36400)  4027!; MIN I=2436748.37+
              +2.82220D*E (J.D.2436380-750)  3732!; OCE/SINCE
              J.D.2441500-CM.TA./SEE TABLE.
EX     VUL    D=0.03P.
EY     VUL    HA MIN II/THE DEPTH OF MIN II 0.05M.
FG     VUL    CM./SEE BB VUL.
              BEA/STAR 120.
              AHA OXA MIN ECKA./THE EPOCH OF LIGHT MINIMUM
              IS GIVEN.
FH     VUL    P VAR. EMEHT, AHHE B TAE, CPABEB
              OCE J.D.2436000./THE ELEMENTS GIVEN IN THE
              TABLE ARE VALID SINCE J.D.2436000.
FK     VUL    EKT AKO./BLAZHKO EFFECT.
FM     VUL    MIN II 13.0.
FN     VUL    D=0.02P; MIN II 14.2.
FP     VUL    MIN II 15.6.
FQ     VUL    MIN II 12.9. BPAEHE H AC C P=280 ET.
              CPABEHE OEATOK B  4248! CM. B  4244!./APSI-
              DAL MOTION WITH P=280 YEARS. CORRECTION OF MISPINTS
              IN  4248! SEE IN  4244!.
FR     VUL    BOMOHO, EPO CEET BOT./PROBABLY THE
              PERIOD MUST BE DOUBLED.
FS     VUL    MIN II 15.2.
FU     VUL    SP KOMOHEHT TECHO AP/SP COMPONENT OF A CLO-
              SE PAIR.
FW     VUL    MIN II 12.9.
FY     VUL    CM./SEE FU VUL.
              K/CYCLE 30-70D  4027!.
FZ     VUL    MIN II 13.9.
GG     VUL    P VAR. MAX=2427681.0+106.5D*E (J.D.2427500-
              28850); OCE/SINCE J.D.2428850-CM.TA./SEE
              TABLE.
GH     VUL    P=2.5D?
GI     VUL    MIN II 13.8.
GK     VUL    KPACHA./RED.
GN     VUL    MIN II 12.4; D=0.04P.
GO     VUL    MIN II-MIN I=0.515P. HA MIN II/THE DEPTH OF
              MIN II 0.03M.
GP     VUL    MIN II 11.2; MIN II-MIN I=0.48P.
GQ     VUL    NF KOMOHEHT TECHO TPOHO P BE./NF
              COMPONENT OF A CLOSE TRIPLE GROUP OF STARS.
              P VAR. MAX=2434399.825+12.647241D*E (J.D.
              2426100-38000)  4414!; OCE/SINCE J.D.2444600-
              CM.TA./SEE TABLE.
GR     VUL    MIN II 13.3.
GT     VUL    MIN II 15.8.
GU     VUL    MIN II 12.2.
GV     VUL    CM./SEE FR VUL.
HI     VUL    MIN II 12.6.
HP     VUL    HA MIN II/THE DEPTH OF MIN II 0.04M.
HS     VUL    MIN II 14.2.
HU     VUL    EKT AKO?/BLAZHKO EFFECT?
HV     VUL    P VAR. MAX=2437165.449+0.419906D*E (J.D.2437100-
              38670); OCE/SINCE J.D.2438670-CM.TA./SEE
              TABLE.
              CM./SEE HU VUL.
HW     VUL    P VAR. MAX=2429077.0+75.44D*E (J.D.2427190-
              29080), MAX=2429077.0+73.94D*E (J.D.2429070-
              32470); OCE/SINCE J.D.2432350-CM.TA./SEE
              TABLE.
IU     VUL    P VAR. MAX=2434656+320.2D*E (J.D.2432700-
              37860)  4427!; OCE/SINCE J.D.2437860-CM.TA./
              SEE TABLE.
IW     VUL    MIN II 13.1.
KN     VUL    MIN II 13.4.
KO     VUL    KPACHA./RED.
KS     VUL    OEH KPACHA./VERY RED.
LT     VUL    MTEPOHOCT:/MULTIPERIODICITY:
              P1=0.109414D, A1(V)=0.0234M; P2=0.11094D,
              A2(V)=0.0074M; P3=0.1215D, A3(V)=0.0070M
              (J.D.2444054-096)  10173!;
              P1=0.109621D, A1(B)=0.0340M; P2=0.093528D,
              A2(B)=0.0136M (J.D.2444071-465)  10193!.
LU     VUL    NOVA VUL 1968 N2.
LV     VUL    NOVA VUL 1968 N1. VB A (B 18M, 6", 115G).
LW     VUL    MIN II 16.3.
MN     VUL    MIN II 16.1; MIN II-MIN I=0.518P; DII=0.10P.
MO     VUL    MIN II 14.8. P VAR?
MR     VUL    P2=111.0D?
MT     VUL    MTEPOHOCT/MULTIPERIODICITY:
              P2=119.93D (A2=0.3M), P3=25.02D (A3=0.4M:).
MX     VUL    P=181.8D?
NO     VUL    MIN II 14.1.
NS     VUL    VB A (B 8.8M, A0, 0.73", 273G, 1978.6), AH PEE-
               MEHEH CMMAPHOO ECKA./THE RANGE OF
              COMBINED LIGHT VARIATION IS GIVEN.
PS     VUL    VB A (B 10.0M, 0.4", 105G, 1980.0); SB 2.
PT     VUL    P1=256.12714S (A1=1.14%), MAX1=
              =2445166.660914 HJED; P2=256.33205S (A2=1.09%),
              MAX2=2445166.659424 HJED; P3=128.11496S (A3=
              =0.37%), MAX3=2445166.660024 HJED.
              MU=0.1508", P=1.6G.
PU     VUL    O BCK SP M4 (1958 .). B 1977-79 .-OCTE-
              EHH O'EM ECKA O 8.7M V; B 1979 . A=0.29M V,
              MIN I=2443943.39+78.12D*E  10197!. B MAX 1979 .
              SP F5IA-:F8-9I. B EBPAE 1980 . ECK HAA
              PEKO AAT  OCT V=13.65M B HAAE CEHTP.
              K CEHTP 1981 . BEA BA  OKOO
              MIN, POOABEOC 500D. B MIN 1980-81 .
              SP M5 C OOCAM TIO, MCCM HALFA, NA D,  OII!,
              FEII, PEKOEMEHX EMEHTOB. B 1982-84 .
              8.35M-8.87M V, SP CHOBA CTA F. OECK PE-
              CTPPOBAC MCC HALFA, HBETA, ACTO C PO-
              M TA P CYG./PRE-OUTBURST SP M4 (1958). GRADUAL
              LIGHT INCREASE IN 1977-79 UP TO 8.7M V; IN 1979 A=
              =0.29M V, MIN I=2443943.39+78.12D*E  10197!. IN
              THE MAX OF 1979 SP F5 IA-:F8-9I. IN FEBRUARY 1980
              AN ABRUPT LIGHT DECREASE STARTED; THE STAR REACHED
              V=13.65M BY EARLY SEPTEMBER. BY SEPTEMBER, 1981
              THE STAR RECOVERED FROM THE DEEP MIN OF 500D DURATION.
              DURING THE 1980-81 MINIMUM SP M5 WITH TIO BANDS,
              EMISSIONS OF HALFA, NAD,  OII!, FEII, RARE EARTHS. IN
              1982-84 8.35M-8.87M V, SP BECAME F AGAIN. SIMETI-
              MES HALFA, HBETA EMISSIONS HAVE BEEN DETECTED, OFTEN
              WITH P CYG PROFILES.
