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IAUC 4872: 1989w; X0331+53

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                                                Circular No. 4872
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
Postal Address: Central Bureau for Astronomical Telegrams
Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Telephone 617-495-7244/7440/7444 (for emergency use only)
TWX 710-320-6842 ASTROGRAM CAM     EASYLINK 62794505
MARSDEN or GREEN@CFA.BITNET    MARSDEN or GREEN@CFAPS2.SPAN


COMET HELIN-ROMAN-ALU (1989w)
     Eleanor F. Helin reports her discovery with Brian P. Roman
and Jeff Alu of another comet with the 0.46-m Schmidt telescope
at Palomar.  R. Bambery assisted.  The object is diffuse with
some condensation.  The following measurements are by Roman:

     1989 UT             R.A. (1950) Decl.        m1
     Oct.  2.41510    2 00 24.26   + 2 17 44.3
           2.43698    2 00 23.54   + 2 17 39.4   17.5
           5.41545    1 58 49.08   + 2 09 30.3
           6.33941    1 58 18.79   + 2 06 57.1
           6.37483    1 58 17.57   + 2 06 52.5

     The following preliminary parabolic elements are from the
above observations; it is likely that this is a short-period comet:

     T = 1989 Apr. 20.482 ET          Peri. = 226.759
                                      Node  =  97.509   1950.0
     q = 2.22413 AU                   Incl. =   6.471

     1989 ET      R.A. (1950) Decl.     Delta      r       m1
     Oct.  1     2 01.12    + 2 21.7    1.941    2.886    17.5
           6     1 58.50    + 2 07.9
          11     1 55.67    + 1 55.0    1.977    2.955    17.7
          16     1 52.73    + 1 43.4
          21     1 49.78    + 1 33.6    2.040    3.027    17.9
          26     1 46.89    + 1 25.9
          31     1 44.17    + 1 20.7    2.130    3.099    18.1


X0331+53
    F. Makino and the Ginga Team, Institute of Space and Astronautical
Science, telex:  "Follow-up observations with the All Sky Monitor
aboard Ginga showed that the transient x-ray source X0331+53 is still
in a bright state (IAUC 4858).  The x-ray intensity in 2-20 keV
remained at 0.3 Crab from Sept. 21 through Oct. 1.  A clear absorption
feature, presumably due to cyclotron resonance, was discovered at
about 29 keV in the x-ray spectra taken with the Large Area Counters."


1989 October 6                 (4872)             Daniel W. E. Green

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