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IAUC 4932: 1989g1; 1989N

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IAUC number


                                              Circular No. 4932
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


PERIODIC COMET RUSSELL 4 (1989g1)
     J. Gibson, OAO Corporation and Jet Propulsion Laboratory,
reports his recovery of this comet with the Palomar 1.5-m
reflector (+ CCD + Gunn r filter), as indicated below.  The
object is stellar within the limits of seeing.

     1989 UT             R.A. (1950) Decl.        m2
     Dec. 11.35311    7 31 03.33   +26 20 51.1    19
          11.36774    7 31 02.93   +26 20 55.2
          11.38325    7 31 02.53   +26 20 59.0
          11.40928    7 31 01.81   +26 21 05.7
          12.36030    7 30 37.44   +26 25 12.4
          12.36612    7 30 37.28   +26 25 13.7
          12.38179    7 30 36.84   +26 25 17.8
          12.39352    7 30 36.54   +26 25 21.1

     The above observations indicate that the prediction on
MPC 12136 (ephemeris on MPC 15430) requires a correction by
Delta(T) = -0.6 day.  Improved orbital elements by B. G.
Marsden, Center for Astrophysics, from 49 observations,
1984-1989 (mean residual 1".2):

                    Epoch = 1990 July  8.0 ET
     T = 1990 July  6.8305 ET         Peri. =  92.9874
     e = 0.366319                     Node  =  70.3963  1950.0
     q = 2.222186 AU                  Incl. =   6.1896
       a =  3.506791 AU    n = 0.1500857    P =   6.567 years


SUPERNOVA 1989N IN NGC 3646
      R. Lopez, University of Barcelona; and A. Riera and J. Cepa,
Instituto de Astrofisica de Canarias, communicate:  "Low-resolution
spectra taken on Dec. 22 with the Faint Object Spectrograph (range
480-970 nm) on the 4.2-m William Herschel Telescope at the position
given by Mikolajczak (IAUC 4823) indicate that SN 1989N is a type-II
supernova, as inferred from the well-defined H-alpha (656.3 nm)
P-Cyg profile.  From this feature, we estimate an expansion velocity
of 6700 km/s.  Fe II (620 nm) and Ca II (857.9 nm) are also present."


1989 December 29               (4932)             Daniel W. E. Green

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