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IAUC 4133: 1985m; CoD -35 11760 AND CPD -58 2721

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                                                  Circular No. 4133
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
Postal Address: Central Bureau for Astronomical Telegrams
Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
TWX 710-320-6842 ASTROGRAM CAM    Telephone 617-495-7244/7440/7444


COMET THIELE (1985m)
     Parabolic orbital elements from MPC 10 156:

         T = 1985 Dec. 18.6627 ET  Peri. =  52.6457
                                   Node  =  52.3569   1950.0
         q =   1.320004 AU         Incl. = 139.1408

     1985/86 ET  R.A. (1950.0) Decl.      p        r       m1

     Nov. 11    23 44.72    +36 23.0    0.565    1.434     7.8
          16    22 45.08    +30 14.6
          21    22 07.75    +24 49.7    0.765    1.383     8.3
          26    21 43.97    +20 39.1
     Dec.  1    21 28.20    +17 31.6    1.031    1.346     8.9
           6    21 17.34    +15 10.9
          11    21 09.64    +13 24.1    1.305    1.325     9.3
          16    21 04.06    +12 02.0
          21    20 59.94    +10 58.2    1.566    1.320     9.7
          26    20 56.85    +10 08.2
          31    20 54.52    + 9 29.2    1.799    1.333    10.0
     Jan.  5    20 52.75    + 8 58.7
          10    20 51.41    + 8 35.3    1.999    1.361    10.3

     Total visual magnitude estimates: Oct. 26.16 UT, 8.6 (J.-C.
Merlin, Le Creusot, France, 0.40-m reflector); Nov. 2.17, 7.7
(C. S. Morris, Palmdale, CA, 20 x 80 binoculars); 6.21, 8.9
(C. E. Spratt, Victoria, BC, 0.20-m reflector); 7.23, 7.7 (Morris,
near Mount Wilson, CA, coma diameter 16').


CoD -35 11760 AND CPD -58 2721
     A. U. Landolt, Louisiana State University, reports that the
extreme-He star CoD -35 11760 = HDE 320156 = LSS 4300 varies in
light and color with an amplitude >= 0.1 mag in V, B-V and U-B.
These data, based on observations made with Cerro Tololo
telescopes over the past seven years, indicate a maximum change in
brightness in a time interval as short as one day.  Observers are
urged to follow this star spectroscopically, since it is suspected
to be a binary (Schonberner and Drilling 1984, Ap.J. 276, 229).
Landolt adds that his photometry of the extreme-He star CPD
-58 2721 = LSS 1922 over the past several years confirm the light
variations announced by Hill et al. (IAUC 4097).


1985 November 12               (4133)              Brian G. Marsden

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