THE ASTRONOMER Electronic Circular No 536       1991 June 4 19.59UT
Ed:Guy M Hurst, 16,Westminster Close, Kempshott Rise,  Basingstoke,
Hants, RG22 4PP, England. Telephone:  (0256)471074 Int:+44256471074
Telex: 9312111261 Answerback: TA G                     JANET BOXES:
GMH at UK.AC.CAM.ASTRONOMY.STARLINK or GUYH at UK.AC.SUSSEX.CLUSTER
TELECOM GOLD: 10074:MIK2885                       PRESTEL 256471074
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COMET LEVY (1991q)
Further precise positions:
     1991 UT             R.A. (1950) Decl.       Observer
     June 17.44271    1 56 08.88   +15 42 17.7   Helin
          17.45660    1 56 12.66   +15 42 52.5     "
          19.06875    2 03 36.00   +16 53 46.5   Vagnozzi
          25.83166    2 35 25.40   +21 37 18.6   McNaught
E. Helin, K. Lawrence, P. Rose, and J. Alu (Palomar).  0.46-m
Schmidt telescope.  Remeasurement of positions given on IAUC 5293.
A. Vagnozzi (Santa Lucia Stroncone).  Communicated by G. Forti.
R. H. McNaught (Siding Spring).  Uppsala Southern Schmidt
telescope.
Preliminary parabolic orbital elements by the undersigned from
nine observations, June 14-25:
     T = 1991 July  7.670 ET          Peri. =  40.741
                                      Node  = 329.596   1950.0
     q = 0.99597 AU                   Incl. =  19.232
IAUC 5296
Ephemeris by Hurst using a program by Nick James:
m =  7.5 + 5.0 log R + 10.0 log r
  Date    R.A. (1950) Dec.     R       r     Elong  Mag.    Motion
          h  m       o  '     (AU)    (AU)     o          "/hr P.A.
1991 July
   4.00   3 15.34  +26 38.0   1.333   0.998   48.0   8.1   186   63
   5.00   3 20.32  +27 11.0   1.337   0.997   47.8   8.1   185   64
   6.00   3 25.31  +27 43.1   1.343   0.996   47.5   8.1   184   64
   7.00   3 30.30  +28 14.3   1.348   0.996   47.3   8.1   182   65
   8.00   3 35.31  +28 44.6   1.354   0.996   47.1   8.1   181   66
   9.00   3 40.33  +29 13.9   1.359   0.996   46.9   8.2   179   66
  10.00   3 45.36  +29 42.3   1.365   0.997   46.7   8.2   178   67
  11.00   3 50.38  +30  9.7   1.371   0.998   46.5   8.2   176   68
  12.00   3 55.41  +30 36.2   1.378   0.999   46.3   8.2   175   68
  13.00   4  0.44  +31  1.7   1.384   1.000   46.2   8.2   173   69
  14.00   4  5.47  +31 26.2   1.391   1.002   46.0   8.2   172   69
  15.00   4 10.49  +31 49.8   1.398   1.004   45.9   8.2   170   70
  16.00   4 15.51  +32 12.4   1.405   1.006   45.7   8.3   168   71
  17.00   4 20.52  +32 34.0   1.412   1.009   45.6   8.3   167   71
  18.00   4 25.52  +32 54.7   1.419   1.012   45.5   8.3   165   72
  19.00   4 30.50  +33 14.4   1.427   1.015   45.3   8.3   163   73
  20.00   4 35.47  +33 33.2   1.434   1.018   45.2   8.4   162   74
  21.00   4 40.42  +33 51.0   1.442   1.022   45.1   8.4   160   74
  22.00   4 45.35  +34  7.9   1.449   1.026   45.1   8.4   158   75
  23.00   4 50.26  +34 23.9   1.457   1.030   45.0   8.4   157   76
  24.00   4 55.14  +34 39.0   1.465   1.035   44.9   8.5   155   76
  25.00   5  0.00  +34 53.2   1.473   1.039   44.9   8.5   153   77
  26.00   5  4.84  +35  6.6   1.481   1.044   44.8   8.5   151   78
  27.00   5  9.64  +35 19.1   1.489   1.050   44.8   8.6   150   78
  28.00   5 14.41  +35 30.8   1.497   1.055   44.8   8.6   148   79
  29.00   5 19.15  +35 41.6   1.505   1.061   44.7   8.6   146   80
  30.00   5 23.85  +35 51.7   1.513   1.067   44.7   8.7   144   80
  31.00   5 28.51  +36  1.0   1.522   1.073   44.7   8.7   143   81

IUE Campaign
Thanks to all observers who contributed to the dwarf nova campaign
during June. Janet Drew in Oxford tells us that our alerts relating
to AH Herculis were the earliest received and permitted this star
to be selected for monitoring by the IUE

Guy M Hurst