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Circular No. 8321 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 C/2004 DZ_61 (CATALINA-LINEAR) An apparently asteroidal object reported independently by the Catalina and LINEAR surveys (discovery observations below from MPEC 2004-E02 and MPS 100749) has been found to have a 4"-diameter centrally condensed coma and a faint tail in p.a. 190-220 deg on R- band CCD images taken on Mar. 16 and 17 UT by S. S. Sheppard, Y. R. Fernandez, and D. Jewitt with the University of Hawaii 2.2-m reflector at Mauna Kea. 2004 UT R.A. (2000) Decl. Mag. Observer Feb. 18.45275 12 37 20.26 - 1 52 38.3 19.3 Catalina 19.37483 12 37 19.80 - 1 19 43.6 19.3 LINEAR Additional astrometry, the following elliptical orbital elements (P = 308 yr), and an ephemeris appear on MPEC 2004-G34. Epoch = 2004 June 4.0 TT T = 2004 May 26.8576 TT Peri. = 44.4612 e = 0.955901 Node = 172.7922 2000.0 q = 2.013352 AU Incl. = 66.8102 SUPERNOVA 2004bi IN UGC 5894 Further to IAUC 8317, K. Shimasaki and W. Li report the LOSS discovery, on KAIT images taken on Apr. 13.23 and 14.20 UT, of an apparent supernova (mag about 18.7) located at R.A. = 10h47m37s.45, Decl. = +26o18'12".0 (equinox 2000.0), which is 25".8 west and 32".1 north of the nucleus of UGC 5894. A KAIT image taken on Mar. 15.25 showed nothing at this position (limiting mag about 19.8). SUPERNOVA 2004bg IN UGC 6363 T. Matheson, P. Challis, and R. Kirshner, Harvard-Smithsonian Center for Astrophysics, report that a spectrum (range 370-750 nm) of SN 2004bg (cf. IAUC 8317), obtained by P. Berlind on Apr. 11.39 UT with the Mt. Hopkins 1.5-m telescope (+ FAST spectrograph), shows it to be a type-Ia supernova near maximum. Adopting the NASA/IPAC Extragalactic Database recession velocity of 6306 km/s for the host galaxy, the supernova expansion velocity is 10600 km/s for Si II (rest 635.5 nm). The spectral-feature age of the supernova (Riess et al. 1997, A.J. 114, 722) is 3 +/- 2 days before maximum light. (C) Copyright 2004 CBAT 2004 April 14 (8321) Daniel W. E. Green
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