Circular No. 2888 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. Cable Address: SATELLITES, NEWYORK Western Union: RAPID SATELLITE CAMBMASS POSSIBLE SUPERNOVA IN NGC 4298 V. P. Dzhapiashvili, Abastumani Astrophysical Observatory, and D. Ya. Martynov, Sternberg Astronomical Institute, report that Natsvlichvili discovered a possible supernova of photographic magnitude 15.0 on Dec. 8 located 10" east and 10" north of the nucleus of NGC 4298 (R.A. = 12h19m.0, Decl. = +14o53', equinox 1950.0). X PERSEI W. Liller, Center for Astrophysics, Harvard and Smithsonian Observatories, reports that he monitored X Per photoelectrically for approximately one hour on both Nov. 11 and 12 using a narrow-band interference filter (full width at peak transmission 15.7 A) centered on He II 4686 A. When the data from both nights are folded modulo 13.924 min (cf. IAUC 2854, 2869), they show a double sine curve with a full amplitude of 0.89 +/- 0.10 percent and with a maximum occurring on Nov. 11d08h18m02s +/- 32s UT. This periodic variation is seen equally well on the two nights although the equivalent width of the He II line, which normally appears in absorption in X Per, is somewhat greater on the first niqht than on the second. COMET SUZUKI-SAIGUSA-MORI (1975k) J. Hers, Randburg, sends the following precise positions: 1975 UT R. A. (1950) Decl. Nov. 29.83333 22 00 24.10 -51 28 14.9 Dec. 2.78403 22 04 29.53 -51 12 54.8 7.77500 22 10 42.65 -50 50 05.6 Selected total visual magnitude estimates: Nov. 11.40 UT, 7.5 (A. F. Jones, Nelson, New Zealand, 4.5-cm refractor); 12.42, 7.8 (Jones); 21.44, 8.8 (L. Boethin, Bangued, The Philippines, 20-cm reflector); 22.45, 8.8 (Boethin); 29.46, 11: (V. L. Matchett, Indooroopilly, Queensland, 30-cm reflector); 30.42, 11: (Matchett). OBSERVATIONS OF COMETS Corrigendum. On IAUC 2681, the observations of comets 1971 VI, 1972 II and 1973f (= 1973 XII) were made at Cerro El Roble, not at Cerro Calan. 1975 December 19 (2888) Brian G. Marsden
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