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Circular No. 8195 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/2003 R1 (LINEAR) An apparently asteroidal object reported by LINEAR (discovery observation below), and posted on the NEO Confirmation Page, has been reported to have cometary appearance on CCD images obtained by J. Ticha and M. Tichy (Klet, 1.06-m KLENOT telescope; slightly diffuse object with a 6" coma on Sept. 5.08 UT, and asymmetric coma to the northwest on Sept. 6.05); and by J. E. McGaha (Tucson, AZ, 0.30-m f/10.0 Schmidt-Cassegrain reflector; 3" coma with a fan- shaped tail 8" long in p.a. 320 deg on Sept. 6.39). 2003 UT R.A. (2000) Decl. Mag. Sept. 2.36756 3 26 08.86 - 1 31 55.5 18.3 The available astrometry, the following preliminary parabolic orbital elements, and an ephemeris appear on MPEC 2003-R35. T = 2003 July 9.968 TT Peri. = 306.497 Node = 356.282 2000.0 q = 2.15420 AU Incl. = 149.675 POSSIBLE NOVA IN M33 M. Ganeshalingam and W. Li, University of California at Berkeley report the discovery via LOTOSS (cf. IAUC 8192) of an apparent nova on unfiltered KAIT images on Sept. 1.4 (mag about 16.9), 4.4 (mag about 17.0), and 6.4 UT (mag about 17.1). The nova is located at R.A. = 1h33m51s.16, Decl. = +30o39'50".2 (equinox 2000.0), which is 3".3 east and 14".4 north of the nucleus of M33 (= NGC 598). A KAIT image taken on Aug. 24.4 showed nothing at this position (limiting mag about 19.5). CORRIGENDA On IAUC 8172, SUPERNOVA 2003gt IN NGC 6930, line 5, FOR 4".7 south READ 9".7 south On IAUC 8188, epsilon INDI B, final sentence, the numbers are simple brightness ratios, as a fraction of the brightness of epsilon Ind B, not as a percentage of the brightness of epsilon Ind B. (C) Copyright 2003 CBAT 2003 September 6 (8195) Daniel W. E. Green
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