Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 6980: 1998de; 1998dh; C/1997 J2; SGR 1627-41

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 6979  SEARCH Read IAUC 6981

View IAUC 6980 in .dvi or .ps format.
IAUC number


                                                 Circular No. 6980
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
Mailstop 18, 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)
URL http://cfa-www.harvard.edu/iau/cbat.html
Phone 617-495-7244/7440/7444 (for emergency use only)


SUPERNOVA 1998de IN NGC 252
     P. Garnavich, S. Jha, and R. Kirshner, Harvard-Smithsonian
Center for Astrophysics, report that a spectrum of SN 1998de (cf.
IAUC 6977) was obtained with the Tillinghast 1.5-m telescope on
July 25.4 UT by M. Calkins.  A broad absorption feature of Si II is
seen at 618.5 nm, implying that this is a type-Ia supernova.
Correcting for the host-galaxy redshift of 5023 km/s (from the NASA
Extragalactic Database), the photospheric expansion velocity is
13 300 km/s.  The blue end of the spectrum shows Ti II absorption,
characteristic of the sub-luminous SNe 1991bg and 1986G, and the
very strong Si II at 580 nm also suggests that this will be a fast-
declining type-Ia event.


SUPERNOVA 1998dh IN NGC 7541
     Garnavich et al. also write:  "A spectrum of SN 1998dh (cf.
IAUC 6978) was obtained with the Tillinghast 1.5-m telescope on
July 26.4 UT by P. Berlind.  The spectrum is clearly that of a
normal type-Ia supernova before maximum.  Broad Si II is observed
at 613.21 nm, implying a photospheric velocity of 13 400 km/s
(assuming a redshift for the host galaxy of 2678 km/s from the NASA
Extragalactic Database).  Interstellar absorption lines of Na I are
seen from our galaxy with an equivalent width (EW) of 0.1 nm and
from NGC 7541 with an EW of 0.04 nm.  SN 1998dh should reach a
visual magnitude of about 13.8."


COMET C/1997 J2 (MEUNIER-DUPOUY)
     Total visual magnitude estimates:  June 20.37 UT, 11.7 (R.
Keen, Mt. Thorodin, CO, 0.32-m reflector); 28.44, 11.4 (N. Biver,
Oahu, HI, 0.26-m reflector); July 2.90, 10.8 (K. Hornoch,
Lelekovice, Czech Republic, 0.35-m reflector); 16.95, 11.6 (R. J.
Bouma, Groningen, The Netherlands, 0.25-m reflector); 19.16, 10.9
(J. Bortle, Stormville, NY, 0.41-m reflector); 22.98, 11.3 (A.
Baransky, Kiev, Ukraine, 0.20-m reflector); 26.90, 10.9 (M.
Reszelski, Szamotuly, Poland, 0.25-m reflector).


SGR 1627-41
     Corrigendum.  IAUC 6962 titled this object incorrectly.

                      (C) Copyright 1998 CBAT
1998 July 27                   (6980)            Daniel W. E. Green

Read IAUC 6979  SEARCH Read IAUC 6981

View IAUC 6980 in .dvi or .ps format.


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


Valid HTML 4.01!