------------------------------------------------------------------- THE ASTRONOMER Electronic Circular No 1301 1998 May 18 20.43UT 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 1998bt L. Germany reports that the Mount Stromlo Abell Cluster Supernova Search Team has discovered an apparent supernova (V = 19.7), presumably associated with the Abell cluster 1736, on V and R CCD images taken on Mar. 10 with the Mount Stromlo 1.27-m telescope (+ Macho Camera). No background host galaxy has been identified for the object, which is located at: R.A. = 13h25m41s.93, Decl. = -26o46'55".7 (equinox 2000.0). SN 1998bt is present on images taken on Feb. 23 and Apr. 6, 18, and 30, with limiting V magnitudes of 21.0, 21.0, 21.5, and 21.5, respectively. The object increased in brightness by > 1.5 mag between Feb. 23 and Apr. 6, and has faded by about half a magnitude since then. The star was not present on an image taken on Jan. 27 (limiting mag V = 21.5). IAUC 6898 SUPERNOVA 1998bv IN HS 1035+4758 A. Yu. Kniazev and N. Arkhyz, Special Astrophysical Observatory (SAO), Russian Academy of Sciences; D. Engels, Hamburger Sternwarte; S. A. Pustilnik and A. V. Ugryumov, SAO; and J. Masegosa, Institute de Astrofizica de Andalucia, Granada, report their discovery of a supernova located 3".1 west and 3".7 south of the emission-line galaxy HS 1035+4758 (R.A. = 10h38m25s.71, Decl. =+47o42'36".5, 2000.0), which is a typical blue compact dwarf galaxy (size about 20") with strong H II emission in its central part. The magnitude of SN 1998bv, estimated from the calibrated spectrum of Apr. 6, is B about 17.1; on Apr. 24, a CCD image yielded B = 17.4, B-V = +0.85. IAUC 6900 (extract) SUPERNOVAE 1998bx, 1998by, 1998bz, 1998ca, 1998cb O. Perdereau and N. Regnault, Laboratoire de l'Accelerateur Lineaire, Universite de Paris-Sud, on behalf of the EROS collaboration, report the discovery of five apparent supernovae, discovered in the course of the automated supernova search with the 1-m Marly telescope (+ CCD) at La Silla: SN Date UT R.A. (2000.0) Decl. V Offset 1998bx Apr. 21 11h12m28.05 - 5 58'09.9 19.6 1".2 W, 5" N 1998by Apr. 21 11 25 07.20 - 5 23 15.2 19.5 0".6 E, 0".6 S 1998bz Apr. 24 12 11 05.84 - 5 35 33.8 19.1 near center 1998ca Apr. 24 12 13 29.24 - 6 23 42.0 18.8 7" W, 7" N 1998cb Apr. 28 10 40 16.07 - 6 15 17.2 20.0 2".3 W, 0".8 N IAUC 6904 (extract) COMET C/1998 J1 SOHO Andrew Pearce, Australia e-mails positive sightings of this comet (cf E1298, E1299): 1998 May 16.44UT: m1=3.3, Dia=3', DC=9...20x80B An impressive sight! Intense central condensation appeared distinctly blue-green in colour. Parabolic shaped tail 2 deg long in PA 110 deg with the central condensation at the focus. First 0.5 deg of tail of high surface brightness and visible easily in the bright twilight sky. 1998 May 17.44UT: m1=3.5, Dia=2.5', DC=9...20x80B Comet seen in a slightly darker sky than previous night. A very impressive object reminiscent of C/1995O1 when at similar brightness. 4.0 deg tail easily visible in PA 100 deg Guy M Hurst