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IAUC 4984: 1989e1; 1990G, 1990B

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                                                  Circular No. 4984
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 SKORICHENKO-GEORGE (1989e1)
     Improved parabolic orbital elements from MPC 16205:

     T = 1990 Apr. 11.9389 ET         Peri. = 137.8482
                                      Node  = 279.3118  1950.0
     q = 1.569001 AU                  Incl. =  59.3652

     1990 ET      R.A. (1950) Decl.     Delta      r       m1
     Mar. 30     1 43.24    +42 13.5    2.172    1.579     8.7
     Apr.  4     2 07.03    +41 54.8
           9     2 30.25    +41 23.6    2.219    1.570     8.7
          14     2 52.72    +40 40.7
          19     3 14.30    +39 47.4    2.283    1.572     8.8
          24     3 34.91    +38 45.1
          29     3 54.49    +37 35.4    2.360    1.586     8.9
     May   4     4 13.03    +36 19.5
           9     4 30.56    +34 58.6    2.446    1.612     9.0
          14     4 47.12    +33 33.9
          19     5 02.77    +32 06.2    2.538    1.649     9.2
          24     5 17.57    +30 36.3
          29     5 31.58    +29 04.9    2.631    1.695     9.4

     Total visual magnitude estimates (cf. IAUC 4972):  Mar. 2.82 UT,
8.5 (O. Midtskogen, Tranby, Norway, 0.32-m reflector); 13.15, 9.3 (C.
Spratt, Victoria, BC, 0.20-m reflector); 18.84, 9.2 (H. Mikuz,
Ljubljana, Yugoslavia, 15x80 binoculars); 22.02, 9.2 (J. E. Bortle,
Stormville, NY, 0.32-m reflector); 24.15, 9.0 (C. S. Morris, Pine
Mountain Club, CA, 20x80 binoculars); 26.81, 9.0 (J.-C. Merlin, Le
Creusot, France, 0.15-m reflector).


SUPERNOVAE 1990G AND 1990B
     A. V. Filippenko and J. C. Shields, University of California
at Berkeley, report that spectra (range 390-980 nm, resolution 1-2
nm), obtained on Mar. 25 UT with a CCD spectrograph on the 3-m Shane
telescope at Lick Observatory, confirm that SN 1990G (IAUC 4982) is
of type Ia, roughly 1-2 weeks past maximum.  Also, spectra of the
type-Ib SN 1990B (IAUC 4949, 4953) show that it is beginning to enter
the supernebular phase dominated by strong [Ca II], [O I], and near-
infrared Ca II emission lines.


1990 March 27                  (4984)             Daniel W. E. Green

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