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Circular No. 6694
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/cfa/ps/cbat.html
Phone 617-495-7244/7440/7444 (for emergency use only)
COMET C/1997 N1 (TABUR)
The following precise CCD positions have been reported:
1997 UT R.A. (2000) Decl. m1 Observer
July 4.33101 4 59 27.00 -26 29 44.3 12.5 Holvorcem
4.33852 4 59 30.32 -26 29 34.0 12.7 "
5.79969 5 10 18.94 -25 58 19.0 Garradd
5.82001 5 10 27.95 -25 57 51.6 "
P. R. Holvorcem (Barao Geraldo). 0.20-m f/6.3 reflector.
G. J. Garradd (Loomberah). 0.25-m f/4.1 reflector.
Parabolic orbital elements from 14 observations July 3-5:
T = 1997 Aug. 15.247 TT Peri. = 345.448
Node = 148.240 2000.0
q = 0.38322 AU Incl. = 86.402
1997 TT R. A. (2000) Decl. Delta r Elong. Phase m1
July 1 4 35.46 -27 27.9 1.256 1.136 58.9 50.0 10.0
6 5 11.80 -25 53.8 1.202 1.043 55.3 53.3 9.6
11 5 49.69 -23 36.7 1.166 0.947 50.9 56.4 9.1
16 6 27.84 -20 34.3 1.150 0.850 45.7 58.8 8.6
21 7 04.95 -16 49.8 1.156 0.752 39.8 60.0 8.1
26 7 40.05 -12 29.5 1.182 0.654 33.6 59.1 7.5
31 8 12.64 - 7 39.2 1.225 0.559 26.9 55.1 6.9
SUPERNOVA 1997cu IN ANONYMOUS GALAXY
The Mount Stromlo Abell Cluster Supernova Search Team (cf.
IAUC 6639) reports the discovery of an apparent supernova (V =
18.2, R = 18.0) on CCD images taken on July 4 by S. Sabine at the
Mount Stromlo 1.27-m telescope (+ Macho Camera). SN 1997cu is
located near Abell 3128 at R.A. = 3h29m03s.0, Decl. = -52d41'41"
(equinox 2000.0), within 1" of its high-surface-brightness
host. SN 1997cu was not present on similar frames taken on Feb. 25 to
R = 20. A spectrum (range 360-750 nm) obtained on the MSSSO 2.3-m reflector
+ DBS spectrograph on July 5 reveals that SN 1997cu is of type Ia and
near maximum. The redshift of the host galaxy, measured from several
absorption lines is z = 0.062, coincident with the redshift of Abell
3128 (z = 0.06).
(C) Copyright 1997 CBAT
1997 July 5 (6694) Brian G. Marsden
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