------------------------------------------------------------------- THE ASTRONOMER Electronic Circular No 1346 1998 Oct 20 20.31UT 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 ------------------------------------------------------------------- PROBABLE SUPERNOVA IN UGC 12133 (=Q1998/079) The Central Bureau have requested that further astrometry is obtained for the object reported by Tom Boles on TAEC 1345 issued earlier today to completely rule out the possibility of an uncatalogued asteroid. Given the UK weather looks unfavourable tonight, we would appreciate assistance from overseas. For professionals receiving these circulars we also seek assistance with spectroscopy. NOVA IN M31 M. Papenkova, J. Y. King, E. Halderson, T. Shefler, M. Modjaz, W. D. Li, R. R. Treffers, and A. V. Filippenko, University of California at Berkeley, report their discovery of an apparent nova in M31 (NGC 224) during the course of the Lick Observatory Supernova Search with the 0.8-m Katzman Automatic Imaging Telescope (KAIT). The nova was found and confirmed on unfiltered CCD images taken on Sept. 30.3 (mag about 16.1) and Oct. 1.3 UT (mag about 16.2). The object is located at R.A. = 0h42m49s.9, Decl. = +41o16'48" (2000), which is about 63" east and 39" north of the galaxy nucleus. IAUC 7023 (extract) COMET C/1998 T1 (LINEAR) One of 17 fast-moving asteroidal objects reported by the Lincoln Laboratory Near Earth Asteroid Research Team on Oct. 2 appears to be a long-period comet, according both to the retrograde nature of its orbit and remarks by Y. Ikari (Moriyama, Japan; relayed by S. Nakano) concerning the object's appearance, when he observed it on Oct. 3 and 8 in response to the request in The NEO Confirmation Page. From the more complete information given on MPEC 1998-T15, the discovery position, orbital elements and ephemeris are extracted below: 1998 UT R.A. (2000) Decl. m1 Oct. 2.28667 1 54 23.56 +23 12 36.5 17.6 T = 1999 June 25.625 TT Peri. = 225.855 Node = 153.122 2000.0 q = 1.47639 AU Incl. = 170.188 1998 TT R. A. (2000) Decl. Delta r Elong. Phase m1 Oct. 14 1 29.69 +21 09.2 2.553 3.531 166.4 3.8 15.5 24 1 06.69 +18 49.6 2.456 3.432 166.7 3.8 15.3 Nov. 3 0 43.65 +16 06.1 2.413 3.332 153.9 7.5 15.1 13 0 22.17 +13 11.8 2.420 3.233 138.9 11.6 15.0 23 0 03.47 +10 21.6 2.472 3.133 123.9 15.2 14.9 IAUC 7026 (extract) VARIABLE STAR IN HERCULES E. Halderson, T. Shefler, M. Modjaz, J. Y. King, M. Papenkova, W. D. Li, R. R. Treffers, and A. V. Filippenko, University of California at Berkeley, report their discovery of a (probably cataclysmic) variable star in our own galaxy during the course of the Lick Observatory Supernova Search with the 0.8-m Katzman Automatic Imaging Telescope (KAIT). The variable star was found and confirmed on unfiltered images taken on Oct. 5.2 (mag about 18.0) and 6.2 UT (mag about 17.8). The object is located at R.A. = 18h14m14s.31, Decl. = +30o43'37".0 (2000). IAUC 7026 (extract) Guy M Hurst