Circular No. 3727 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 617-864-5758 1982 RB H.-E. Schuster, European Southern Observatory, provides the following semiaccurate positions, the first three of which replace those on IAUC 3725: 1982 UT R.A. (1950.0) Decl. Mag. Sept. 14.12286 23 04.09 -23 53.8 17 14.16441 23 04.14 -23 56.4 15.11285 23 05.34 -24 51.5 19.29132 23 10.47 -28 27.0 21.07917 23 12.94 -29 49.5 SUPERNOVA IN NGC 1332 D. A. Allen, Anglo-Australian Observatory; and A. Evans, University of Keele, report that this object (cf. IAUC 3684) has formed a dust shell at a temperature of ~ 1100 K. The 2.2-micron (K band) magnitude ~ 14. Information regarding the ejection velocity and the form of the visual light curve is urgently required for a complete interpretation. Evans requests that such information be sent to him at the address: Department of Physics, The University, Keele ST5 5BG, England. 2 CETI AND lambda ERIDANI P. K. Barker, Department of Astronomy, University of Western Ontario, reports his discovery that 2 Cet = HR 9098 is a Be star; H-alpha image-dissector-scanner observations on Sept. 5 show centrally-reversed emission superposed on photospheric absorption. Further, the bright Be star lambda Eri = HR 1679 is entering a new active emission phase; H-alpha observations on Sept. 8 show centrally- reversed emission above the continuum. From 1980 Sept. to 1981 Oct. H-alpha in lambda Eri has shown only broad photospheric absorption. COMET AUSTIN (1982g) Total visual magnitude, coma diameters and tail length estimates by J. Bortle, Stormville, NY: Sept. 4.04 UT, 6.1, 4'.0, - (10x50 binoculars); 6.04, 6.3, 4'.5, - (10x50); 10.05, 6.7, 4', 10' in p.a. 39 (10x50); 12.05, 6.9, 3'.5, 5' in p.a. 35 (10x50); 20.03, 7.8, 4'.2, 5' in p.a. 48 (20x80 binoculars). 1982 September 22 (3727) Brian G. Marsden
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