Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 6380: 1996X; 1996W; C/1995 O1

The following International Astronomical Union Circular may be linked-to from your own Web pages, but must not otherwise be redistributed (see these notes on the conditions under which circulars are made available on our WWW site).


Read IAUC 6379  SEARCH Read IAUC 6381

View IAUC 6380 in .dvi or .ps format.
IAUC number


                                                  Circular No. 6380
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)


SUPERNOVA 1996X IN NGC 5061
     G. J. Garradd, Loomberah, Australia, and S. Nakano, Sumoto,
Japan, report the independent discoveries of an apparent supernova
in NGC 5061 by Robert O. Evans (Coonabarabran, N.S.W., on Apr. 12.5
UT, mag about 13, visual) and by Kesao Takamizawa (Saku-machi,
Nagano-ken, on Apr. 12.618, mag 13.5, T-Max 400 film), respectively.
R. and Y. Kushida (Yatsugatake) report the following precise
position for SN 1996X from a CCD frame exposed on Apr. 13.480: R.A.
= 13h18m01s.13, Decl. = -26o50'45".3 (equinox 2000.0; mag 14.0),
which is about 52" west and 31" south of the galaxy's center.  From
a CCD exposure on Apr. 13.443, Garradd provides a position for the
supernova with position end figures 01s.14, 46".0.  Evans reports
that no object was seen at this position on Mar. 24; Y. Kushida
reports that a patrol film (Technical Pan 6415, limiting mag 15.5)
exposed on 1993 Feb. 24 shows nothing at this position.
Furthermore, no object is present at this location on the digital
sky survey (field taken in May 1976).  A nearby field star of mag
about 16 has position end figures 03s.33, 30".5.


SUPERNOVA 1996W IN NGC 4027
     N. B. Suntzeff reports that spectrophotometry (range 370-730
nm) obtained by M.-T. Ruiz with the Cerro Tololo 4-m telescope on
Apr. 13.1 UT confirms that this is a type-II supernova near maximum
(cf. IAUC 6379), with a very blue continuum.  CCD images were
obtained by D. DePoy with the Cerro Tololo 0.9-m telescope,
yielding the following position (using the digital sky survey) for
SN 1996W:  R.A. = 11h59m28s.98, Decl. = -19o15'21".9 (equinox
2000.0), which is 17" west and 34" north of the nucleus of the
galaxy.  Provisional photometry gives V = 15.1 on Apr. 13.1.


COMET C/1995 O1 (HALE-BOPP)
     Visual m1 and coma-diameter estimates:  Mar. 23.50 UT, 8.6, -
(A. Hale, Cloudcroft, NM, 10x50 binoculars); 27.67, 7.9, - (D.
Seargent, The Entrance, NSW, Australia, 25x100 binoculars); 28.13,
8.5, 2'.6 (M. Plsek, Lelekovice, Czech Republic, 0.35-m reflector);
30.46, 8.2, - (Hale); Apr. 1.77, 7.3, about 8' (Seargent, 10x50
binoculars); 7.09, 8.3, 4'.5 (A. Baransky, Kiev, Ukraine, 0.11-m
reflector).

                      (C) Copyright 1996 CBAT
1996 April 13                  (6380)            Daniel W. E. Green

Read IAUC 6379  SEARCH Read IAUC 6381

View IAUC 6380 in .dvi or .ps format.


Our Web policy. Index to the CBAT/MPC/ICQ pages.


Valid HTML 4.01!