Circular No. 2991 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 SUPERNOVA IN NGC 7117 J. R. Dunlap, Corralitos Observatory, Northwestern University, reports the discovery of a supernova 7" west and 13" south of the nucleus of NGC 7177. The object was estimated at mv = 16.5 on Sept. 28.2 UT, but the brightness was not appreciably different on Sept. 23.2 and 27.2. Supernova 1960L was in the same galaxy. HD 5980 M. W. Feast and A. D. Thackeray, South African Astronomical Observatory, draw attention to the following erratum, published in Monthly Notices Roy. Astron. Soc. (1972) 155, 383, concerning HD 5980 = R14 (cf. IAUC 2989): "In Fig. 3 [of Feast et al. 1960, ibid. 121, 337], the identification of R14 (HD 5980) should refer to the star 6.5 mm to the left of the marked 'star', which is in fact a compact group [HD 5942] surrounded by a faint nebulosity." PERIODIC COMET FAYE (1976i) The following precise positions have been reported: 1976 UT R. A. (1950) Decl. m1 Observer Aug. 20.61181 20 37 55.91 - 4 37 28.0 15.5 Seki 25.87734 20 33 42.66 - 5 11 08.9 16.2 Mrkos 25.89175 20 33 42.01 - 5 11 16.1 " 26.86863 20 32 57.71 - 5 17 46.5 16.0 Vavrova 26.88322 20 32 57.11 - 5 17 54.1 " 28.84757 20 31 31.37 - 5 31 09.3 16.2 Mrkos 28.86198 20 31 30.80 - 5 31 14.8 " T. Seki (Geisei). From Orient. Astron. Assoc. Comet Bull. No. 134. A. Mrkos and Vavrova (Klet Observatory). 1973 EA The following precise position was measured by C. Y. Shao from an exposure by R. E. McCrosky, Harvard Observatory, Agassiz Station: 1975 UT R. A. (1950) Decl. Dec. 1.95928 20 49 26.01 -13 58 20.4 1976 September 30 (2991) Brian G. Marsden
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