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[vsnet-history 546] New Variable Stars Designated in 1992 (Granslo)




Date: Tue, 30 Mar 1993 18:32:24 +0200
From: granslo@argo.uio.no
Subject: New Variable Stars Designated in 1992


            LIST OF VARIABLE STARS FINALLY DESIGNATED IN 1992
            +++++++++++++++++++++++++++++++++++++++++++++++++

This list is extracted from Kazarovetz et al. (1993). We have included
variables with maximum magnitudes of 13.5 or brighter and amplitudes of
0.20 magnitudes or more. These objects may be suitable for visual and
photoelectric photometry using smaller telescopes. Only stars with measure-
ments in the following magnitude systems have been considered: b, B, P, R,
v and V. These systems have spectral responses that mainly fall within the
visual (or near infrared) part of the spectrum.

Coordinates have been precessed to the equinox 2000.0. The types of varia-
bility are according the GCVS classification (Kholopov et al. 1985). Other
names and designations are given under the notes column.

In 1992 438 new variables were finally designated and the total number has
reached 30702.

-----------------------------------------------------------------------------
 Variable   RA (2000.0) Dec    Max   Min      Type    Notes
-----------------------------------------------------------------------------
   NO Aps  17 31 28 -80 51.5   5.71   5.95 V  SR      NSV 8609 = HR 6429
   HS Aqr  20 40 54 - 0 35.8   9.35   9.77 V  EB      SAO 144692 = HD 197010
   HT Aqr  21 40 20 - 1 47.2   9.6   11.0  B  SR      DHK 8 = SAO 145577
V1413 Aql  19 03 47 +16 26.3  10.6   15.1  V  ZAND+E  AS 338
V1414 Aql  19 34 40 - 7 34.3   9.0   14.4  V  M       Wakuda's variable star

Alpha Ara  17 31 50 -49 52.5   2.79   3.13 b  BE      NSV 8999 = HR 6510
   CC Cam   4 57 17 +69 27.2  10.7   14.5  V  M       TAV 0451+69
   EZ Cnc   8 52 57 +23 27.8  11.78  12.72 V  RRAB    NSV 4285
   HS CMa   6 33 41 -18 07.6   9.8   14.0  V  M       Wakuda's star
 V432 Car  11 08 41 -60 42.9  11.79  12.43 V  SDOR    IRAS 11065-6026

 V868 Cen  13 50 11 -63 08.9  10.24 <22.5  V  N       Nova Centauri 1991
   UX CrB  16 16 55 +31 07.0  13.12  13.60 B  EA      1E 1615.0+3114
   TV Crv  12 20 24 -18 27.0  12     18    P  UG      Tombaugh's variable
   CH Cru  12 41 57 -59 41.1   4.88   5.7  B  GCAS:   NSV 5858 = HR 4823
V1964 Cyg  19 30 06 +31 24.2  12.0   12.8  P  SRD:    SVS 2882

V1967 Cyg  19 43 44 +30 08.1   7.43   7.83 V  SRB     NSV 12387 = DHK 12
V1970 Cyg  20 15 51 +46 54.5  11.4   12.3  P  SR      DHK 21 = BD +26 2892
V1972 Cyg  20 23 03 +39 29.8  11.54  12.12 B  IA      MWC 342
V1973 Cyg  20 23 09 +40 50.2   9.67  10.09 V  ISA     HDE 229189
V1974 Cyg  20 30 31 +57 37.9   4.2   17.5: V  NA+E:   Nova Cygni 1992

V1977 Cyg  20 47 37 +43 47.4  10.81  11.44 V  INA     NSV 13308 = AS 442
V1978 Cyg  20 48 56 +33 23.0  13.2   14.2  B  SR      IRAS 20469+3312
V1980 Cyg  21 01 55 +49 51.6  12.29  12.50 V  INT     NSV 13477
V1981 Cyg  21 02 24 +44 47.5   7.5    8.1  B  SRB     HR 8062 = SAO 50381
V1982 Cyg  21 03 54 +50 15.2  12     13.8  B  INT     NSV 13505

V1983 Cyg  21 13 11 +40 11.4  12.26  14.48 V  SR:     BC 45
   EO Dra  18 20 55 +50 30.2  10.8   13.0  P  M:      NSV 10701
   EQ Dra  19 25 16 +57 13.9  10.3   11.6  V  SRB     TASV 1924+57
   EO Eri   4 45 10 -23 51.6  10.3   18.0  P  M       NSV 1710
 V836 Her  18 11 32 +23 55.3  10.7   11.4  V  EA      TASV1809+23 = HDE341703

 V838 Her  18 46 32 +12 14.1   5.0   20    V  NA+EA   Nova Herculis 1991
   WX Hor   3 49 35 -52 04.9   7.14   7.88 V  SRA     NSV 1382 = SAO 233291
   DU Leo   9 44 11 +25 11.3   8.68   9.43 R  EA/SD   DHK 16 = SAO 80992
   DV Leo   9 53 58 +10 15.5   7.78   8.13 V  SR      DHK 15 = SAO 98835
   HV Lup  15 28 17 -45 08.1   7.30   8.09 V  BE:     NSV 7086 = SAO 225814

   BI Lyn   9 03 19 +39 51.0  12.93  13.13 B  NL      PG 0900+401
 V489 Lyr  18 56 41 +28 39.4  13.0   18.3  P  M       SVS 2873
 V694 Mon   7 25 51 - 7 44.1   9.1   10.1  V  *       MWC 560 (symbiotic)
V2264 Oph  17 20 21 -26 46.5   9.8  <21  : V  NA      Nova Ophiuchi 1991
V2288 Oph  17 41 52 + 5 16.3  12.6   13.1  P  EA      NSV 9538

V2290 Oph  17 43 05 -20 07.0   9.3  <22  : V  NA      Nova Oph 1991, No. 2
V1202 Ori   4 56 06 +10 05.7  11.88  12.76 V  EA      NSV 1776 = HV 10400
V1232 Ori   5 35 26 - 5 27.6  11.5   12.9  V  IN      Huruhata No. 1 (1987)
V1258 Ori   5 45 26 - 4 14.4  12.0   12.6  P  SR:     NSV 2622 = DHK 10
   KV Peg  21 22 05 +17 08.3  11.73  11.93 V  EW/KW   1E 2119.7+1655

   KW Peg  21 39 10 +26 42.6  12.1   12.41 V  EA      Comp. star for BX Peg
 V502 Per   2 17 45 +56 54.0   9.36   9.56 V  BE      SAO 23136 (h,kappa Per)
 V503 Per   2 20 39 +57 18.7   9.43   9.72 V  BE      BD+56 548 (h,kappa Per)
 V504 Per   2 21 18 +57 18.1   9.77   9.98 V  BE      BD+56 559 (h,kappa Per)
 V505 Per   2 21 13 +54 30.6   6.87   7.46 V  EA/DM   DHK 11 = SAO 23229

 V506 Per   2 21 44 +57 07.5   9.45   9.69 V  BE      NSV 794 (h,kappa Per)
 V507 Per   2 21 53 +57 07.5   9.77  10.09 V  BE      NSV 796 (h,kappa Per)
 V510 Per   3 13 51 +43 51.9   7.30   7.52 V  RS      SAO 38659 = HD 19942
 V511 Per   3 26 26 +40 27.5   8.1    8.6  V  EA/DM   DHK 9 = SAO 38830
 V513 Per   3 32 32 +41 26.5  10.4   13  : V  M       TAV 0329+41 = CCS 149

Gamma Per   3 04 48 +53 30.4   3.63   4.18 B  EA/GS   23 Per = HR 915
   BE Psc   1 04 07 +26 35.2   8.8    9.0  V  RS      SAO 74467 = HD 6286
 V351 Pup   8 11 38 -35 07.5   6.4  <12    V  NA      Nova Puppis 1991
   VY Pyx   8 54 30 -23 31.4   7.65   8.08 B  CWB     NSV 4298 = SAO 176679
   VZ Pyx   8 59 20 -24 28.9  12.5   16.8  V  UG      1H 0857-242

   WW Pyx   9 04 32 -32 22.6  12.4   13.2  V  E       Comp. star for T Pyx
 V335 Sge  20 14 21 +17 00.9   9.8   11.2  P  SRB     NSV 12930 = DHK 20
V4157 Sgr  18 09 35 -25 52.0   7    <21    V  NA      Nova Sgr 1992, No. 1
V4160 Sgr  18 14 14 -32 12.5   7.0  <21    V  NA      Probable Nova Sgr 1991
V4169 Sgr  18 23 27 -28 22.0   7.7  <12.6  V  NA      Nova Sgr 1992, No. 2

V4171 Sgr  18 23 41 -22 59.5   7.49  20.5: V  NA      Nova Sgr 1992, No. 3
V4197 Sgr  19 05 58 -19 28.9   7.95   8.70 V  EW/KE   NSV 11722 = SAO 162180
 V992 Sco  17 07 18 -43 15.3   7.26  18  : V  NA      Nova Scorpii 1992
 V444 Sct  18 47 10 - 8 20.9  10.5  <20    V  NA      Nova Scuti 1991
   TT Sex   9 46 26 - 6 01.9  10.4   11.9  P  LB      NSV 4621 = DHK 18

V1059 Tau   4 42 55 +25 16.6  13.2   14.5  P  UVN     NSV 1699 = SVS 1099
V1060 Tau   4 50 37 +15 47.0  11.2   12.18 B  LB:     NSV 1737 = DHK 24
V1061 Tau   4 58 53 +24 29.7   7.95   8.45:V  EB/KE   DHK 14 = SAO 76868
   XX Tri   2 03 47 +35 35.5   8.1    8.7  V  RS      SAO 55233 = HD 12545
   LT Vel   8 48 14 -44 52.3   9.95  10.46 V  EB      NSV 4260 = BV 1200

   IK Vir  12 13 57 + 2 00.5  11.51  11.79 V  EA      Feige 58
 V335 Vul  19 23 15 +24 28.3  10.1   12    P  SR      TAV 1921+14 = AS 356
 V336 Vul  19 34 43 +23 53.3   7.7    9.6  V  SRB:    NSV 12178 = DHK 6
-----------------------------------------------------------------------------

References:
----------
Kazarovetz, E. V., Samus, N. N, and Goranskij, V. P.: 1993, "The 71st
  Name-List of Variable Stars", Information Bulletin on Variable Stars,
  No. 3840, Konkoly Observatory, Budapest.
Kholopov, P. N. et al.: 1985, "General Catalogue of Variable Stars", 4th
  Edition, Vol. 1, Nauka, Moscow.

-----------------------------------------------------------------------------
Bjoern Haakon Granslo                               Tel.:    + 47 22 85 65 16
Astrofysisk institutt                                Fax:    + 47 22 85 65 05
Postboks 1029, Blindern                         Internet: granslo@argo.uio.no
N-0315 Oslo, Norway                                 SPAN:       ARGO::GRANSLO
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