------------------------------------------------------------------- THE ASTRONOMER Electronic Circular No 1631 2001 May 10 13.51UT 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 ------------------------------------------------------------------- SUPERNOVA 2001bg IN NGC 2608 (Q2001/216) Tom Boles sent a single image to the editor of NGC 2608 on May 8 showing an apparently new mag 14 object. Although many asteroids were predicted to be in the field, only Sidonia was bright enough to be a candidate but was approximately 15' from the galaxy which was considered unlikely to be due to an error in the orbital elements. An appeal was issued to the TA Checking Group and Heinz Kerner quickly responded with a confirmatory image on May 9. Meanwhile Tom obtained another image on the same date confirming the object had not moved. This has enabled the following IAUC to be issued: Guy M. Hurst, Basingstoke, England, reports the discovery by Tom Boles, Coddenham, of an apparent supernova (mag about 14) on an unfiltered CCD frame (limiting mag about 18) taken on May 8.943 UT with a 0.36-m Schmidt-Cassegrain telescope in the course of the U.K. Nova/Supernova Patrol. The object was near the same brightness on a second image obtained by Boles on May 9.9 in rather poor conditions. The new object is located at R.A. = 8h35m18s.86, Decl. = +28o28'05".8 (2000), which is 22" east and 19" south of the centre of NGC 2608. Nothing appears at this location on a master image taken on 2000 Jan. 13.956 (limiting mag about 19) or on Palomar Sky Survey images taken on 1989 Nov. 8 (limiting red mag about 20) and on 1990 Mar. 23 (limiting blue mag about 20). SN 2001bg also appears near mag 14 on an unfiltered CCD image taken on May 9.884 with a 0.15-m reflector by H. Kerner, Fassberg, Germany, at the request of Hurst. IAUC 7621 Congratulations to Tom Boles on this first supernova from his new observing site at Coddenham and thanks to Heinz Kerner for his valuable confirmation. COMET C/2001 A2 (LINEAR) C. W. Hergenrother, M. Chamberlain, and Y. Chamberlain, Lunar and Planetary Laboratory, University of Arizona, report that 60-s R-band images of C/2001 A2 taken on Apr. 30.12 UT with the Catalina 1.54-m reflector show a double nucleus. The two components are nearly equal in brightness and 3".5 apart and aligned precisely on an east-west line. Both components are highly condensed. Observations (with the same telescope) on Apr. 24.14 show only a single nucleus. IAUC 7616 (extract) EDITORIAL ABSENCE The editor will be absent from tomorrow morning (May 11) and will return the following evening (May 12). During this short interval please send messages to the editor's mailbox but naturally there will be a short delay on my return whilst the backlog is cleared. Discoveries should additionally be reported to Nick James (see magazine for contact details). Guy M Hurst