Circular No. 4506 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. TWX 710-320-6842 ASTROGRAM CAM Telephone 617-495-7244/7440/7444 COMET FURUYAMA (1987f1) Parabolic orbital elements from MPC 12575: T = 1988 Mar. 2.415 ET W = 232.953 O = 250.063 1950.0 q = 1.69121 AU i = 117.851 1987/88 ET R.A. (1950) Decl. Delta r m1 Dec. 1 4 36.93 +18 29.7 1.089 2.073 9.9 6 4 12.22 +13 48.1 11 3 48.09 + 8 53.4 1.061 2.003 9.6 16 3 25.49 + 4 04.4 21 3 05.12 - 0 22.9 1.127 1.938 9.6 26 2 47.32 - 4 18.6 31 2 32.17 - 7 39.9 1.262 1.879 9.7 Jan. 5 2 19.51 -10 28.6 10 2 09.11 -12 48.7 1.435 1.826 9.9 15 2 00.70 -14 45.0 20 1 54.02 -16 21.9 1.622 1.781 10.1 Total visual magnitude estimates: Nov. 28.48 UT, 10.0 (D. Levy, Tucson, AZ, 0.4-m reflector); 29.44, 10.7 (A. Hale, Las Cruces, NM, 0.41-m reflector); Dec. 1.28 UT, 10.0 (R. A. Keen, Mt. Thorodin, CO, 0.15-m reflector). Corrigenda. IAUC 4502, line 3, for 21.79074 read 21.78021; line 16, add S. Hayakawa (YGCO Hoshikawa and Nagano Stations). RZ LEONIS Visual magnitude estimates communicated by J. Mattei, AAVSO: Nov. 25, [12.5 (J. Isles, Limassol, Cyprus); Dec. 1.238 UT, 12.7 (S. Lubbock, Bridgend, Wales). Mattei notes that this does not appear to be a recurrent nova (as listed in the 4th edition of the Variable Star Catalogue) but some sort of long-period dwarf nova. SUPERNOVA 1987A IN THE LARGE MAGELLANIC CLOUD Visual magnitude estimates: Nov. 25.44, 6.0 (D. Seargent, The Entrance, N.S.W.); 26.55, 5.8 (R. H. McNaught, Coonabarabran, N.S.W.); 28.42, 6.1 (Seargent); 29.44, 6.0 (A. C. Beresford, Adelaide, South Australia); 30.44, 6.0 (Beresford); Dec. 1.48, 6.1 (Beresford); 2.44, 6.1 (Seargent); 3.50, 5.9 (McNaught). 1987 December 3 (4506) Brian G. Marsden
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