------------------------------------------------------------------- THE ASTRONOMER Electronic Circular No 1400 1999 Apr 18 14.40UT Ed:Guy M Hurst, 16,Westminster Close, Kempshott Rise, Basingstoke, Hants, RG22 4PP,England.Telephone/FAX(01256)471074Int:+441256471074 INTERNET: GUY@TAHQ.DEMON.CO.UK GMH at AST.STAR.RL.AC.UK WORLD WIDE WEB http://www.demon.co.uk/astronomer ------------------------------------------------------------------- COMET 1999 H1 Steven Lee reports his visual discovery of a comet at a star party near Mudgee, New South Wales. The following observations are available: 1999 UT R.A. (2000) Decl. m1 Observer Apr. 16.5 14.0 -69 9 Lee 16.59549 13 49 24.64 -68 21 33.6 Garradd 16.59650 13 49 23.58 -68 21 33.3 " 16.59941 13 49 20.80 -68 21 32.3 " 16.61689 13 49 03.53 -68 21 26.4 " 16.61777 13 49 02.67 -68 21 26.0 " 16.61839 13 49 02.14 -68 21 25.7 " S. Lee (Mudgee, N.S.W.). Comet diffuse with no visible tail. G. J. Garradd (Loomberah). 0.45-m f/5.4 reflector + CCD. m_2 = 13.9-14.2. Visually, the comet has a 3' coma slightly elongated northward. IAUC 7144 Andrew Pearce, Nedlands, Australia has e-mailed TA to report he has seen this new comet visually: 1999 Apr 17.462UT, m1=9.2, coma diameter 2.0', DC5. 0.41-m reflector. Moderately condensed bright object. He adds that he was observing several variables within about 10-15 degrees of the discovery position on April 16! 1999 Apr 17.765UT, m1=9.1, coma diameter 2.4', DC6. 0.41-m reflector. 1999 GU3 Gary Poyner reports that he has seen this asteroid (cf E1397) visually. On 1999 April 15.000UT, estimated magnitude 14.8 (0.40-m reflector). He adds that it was then near the W CrB (mira) variable star field. SUPERNOVA 1999bu IN NGC 3786 W. D. Li, University of California at Berkeley, on behalf of the Lick Observatory Supernova Search with the 0.8-m Katzman Automatic Imaging Telescope (KAIT), reports the discovery of an apparent supernova in NGC 3786, a Seyfert galaxy that is in a pair of interacting galaxies (Arp 294 and NGC 3788). SN 1999bu was discovered on an unfiltered image taken on Apr. 16.3 UT (mag about 17.5). Inspection of earlier images taken by KAIT reveals that the supernova was barely visible on Mar. 13.3 and clearly present on Mar. 28.3 (mag about 17.6). The new object is located at R.A. = 11h39m42s.50, Decl. = +31o54'29".1 (2000), which is about 1".3 west and 3".1 south of the nucleus of NGC 3786. IAUC 7145 (extract) Guy M Hurst