Read IAUC 8011
.dvi or
.ps format.
Circular No. 8010
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)
CBAT@CFA.HARVARD.EDU (science)
URL http://cfa-www.harvard.edu/iau/cbat.html ISSN 0081-0304
Phone 617-495-7440/7244/7444 (for emergency use only)
COMET 2002 V1
S. Pravdo, Jet Propulsion Laboratory, reports the NEAT
discovery, on CCD images taken with the 1.2-m reflector at
Haleakala, of a comet with a tail about 10" long in p.a. 225 deg.
Following posting on the NEO Confirmation Page, other CCD observers
have confirmed the cometary nature: P. Pravec and L. Sarounova
(Ondrejov, 0.65-m reflector), coma diameter 0'.4, faint tail 0'.4
long in p.a. 250 deg; M. Lehky (Hradec Kralove, Czech Republic,
0.40-m f/5 reflector), slightly diffuse coma of diameter about 5";
M. Blasco and S. Sanchez (Mallorca, 0.40-m Schmidt telescope), coma
diameter 15". Available astrometry:
2002 UT R.A. (2000) Decl. m1 Observer
Nov. 6.59602 5 05 40.42 +16 21 03.0 17.3 NEAT
6.60641 5 05 39.30 +16 21 03.9 17.5 "
6.61673 5 05 38.08 +16 21 03.8 17.1 "
6.82561 5 05 15.90 +16 21 19.8 16.4 Blasco
6.82802 5 05 15.80 +16 21 19.5 16.5 "
6.85041 5 05 13.15 +16 21 21.9 Lehky
6.85525 5 05 12.72 +16 21 22.3 "
6.85850 5 05 12.27 +16 21 21.9 "
6.86370 5 05 11.67 +16 21 22.7 "
6.88959 5 05 09.11 +16 21 24.7 Pravec
6.89146 5 05 08.90 +16 21 24.7 "
6.89348 5 05 08.67 +16 21 24.8 16 "
6.90192 5 05 07.47 +16 21 24.8 Lehky
6.90542 5 05 07.19 +16 21 26.0 "
6.91061 5 05 06.62 +16 21 27.3 "
6.91382 5 05 06.00 +16 21 27.1 "
SUPERNOVA 2002hk IN MCG +07-15-6
A. V. Filippenko, R. Chornock, and S. Jha, University of
California at Berkeley, report that inspection of a CCD spectrum
(range 400-1000 nm) obtained on Nov. 6 UT with the Keck II 10-m
telescope (+ ESI) shows that SN 2002hk (cf. IAUC 8007) is a
somewhat-unusual type-II supernova. Superposed on the relatively
red continuum is a strong, broad H-alpha emission line; weaker Na D
(possibly He I), H-beta with a P-Cyg profile, and several
additional features are also present. The object's spectrum bears
some resemblance to that of SN 2000cs (IAUC 7448).
(C) Copyright 2002 CBAT
2002 November 6 (8010) Daniel W. E. Green
Read IAUC 8011
.dvi or
.ps format.
Our Web policy. Index to the CBAT/MPC/ICQ pages.