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Circular No. 6470
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
Postal Address: Central Bureau for Astronomical Telegrams
Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
IAUSUBS@CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions)
BMARSDEN@CFA.HARVARD.EDU or DGREEN@CFA.HARVARD.EDU (science)
Phone 617-495-7244/7440/7444 (for emergency use only)
COMET 1996 R1
Carl W. Hergenrother, University of Arizona, reports his
discovery of a comet on films taken by Timothy B. Spahr, University
of Florida, and himself at the University of Arizona's site east of
Tucson. The following observations are available:
1996 UT R.A. (2000) Decl. m1 Observer
Sept. 7.28437 0 00 12.45 +39 20 45.8 14 Hergenrother
7.31296 0 00 00.49 +39 19 25.7 "
8.13036 23 54 03.58 +38 38 45.7 "
8.36182 23 52 21.78 +38 26 55.9 13.4 Offutt
8.36434 23 52 20.67 +38 26 47.8 13.2 "
8.36612 23 52 19.87 +38 26 42.0 13.2 "
8.36873 23 52 18.73 +38 26 33.6 13.0 "
8.37292 23 52 16.91 +38 26 21.2 13.2 "
8.37875 23 52 14.26 +38 26 03.4 Hergenrother
8.38361 23 52 12.17 +38 25 48.6 "
C. W. Hergenrother and T. B. Spahr (Mount Bigelow). 0.41-m f/3
Schmidt. Comet well condensed, faint tail extending a few arcmin
to the south. Their visual estimates on Sept. 8 suggest m1 about
11-12.
W. Offutt (Cloudcroft). 0.6-m f/7 Ritchey-Chretien + CCD. Roughly
circular coma about 4'.25 across with 35" condensation. No tail
on 60-second exposures.
SUPERNOVA 1986P IN NGC 5763
J. Mueller reports her discovery of an apparent supernova of
mag about 17 on a IIIa-J plate taken with the 1.2-m Oschin Schmidt
Telescope on 1986 July 2 by E. Helin and Mueller in the course of
the second Palomar Sky Survey. The candidate is located 8" west
and 6" south of the center of NGC 5763 (R.A. = 14h49m.0, Decl. =
+12 29', equinox 2000.0). A Palomar J plate taken on 1993 Mar. 3
by C. Brewer and Mueller shows nothing at the position; N. Reid
also reports that an F plate taken on 1986 June 13 by W. Sargent
and Mueller shows no object at the position, indicating the
apparent supernova was < 3 weeks old when photographed. The image
quality corresponds to nearby images indicating that it is very
unlikely that the object is asteroidal in nature or a plate defect.
(C) Copyright 1996 CBAT
1996 September 8 (6470) Daniel W. E. Green
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