Circular No. 4375 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 SUPERNOVA 1987G IN UGC 7370 J. Mould and R. Day report their discovery of a magnitude 15 supernova in UGC 7370 (MCG +0-32-01; R.A. = 12h17.2, Decl. = +2 22', equinox 1950.0) on a plate exposed Apr. 25.25 UT with the 1.2-m Schmidt telescope during the course of the second Palomar Sky Survey. The supernova is located about 30" from the center of the galaxy along the southeast semimajor axis (p.a. 151 deg). Observations on Apr. 26 by J. Gunn, M. Schmidt, and D. Schneider with the 5-m Hale telescope (+ 4-shooter) indicate no noticeable magnitude change in one day and also that the object has a possible type-I SN spectrum. SUPERNOVAE 1987C AND 1987D R. P. Kirshner and E. M. Schlegel, Center for Astrophysics, report that spectra, obtained by J. Huchra and R. C. Smith at the Multiple Mirror Telescope, of SN 1987C (IAUC 4358, 4368) and SN 1987D (IAUC 4370) show that SN 1987C is an old type-II object, while SN 1987D is type I. COMET WILSON (1986l) J. R. Ducati and R. D. D. Costa, Instituto de Fisica, Porto Alegre, telex: "We report photoelectric photometry of comet Wilson on Apr. 23.38, 24.39, and 25.40 UT with the Lowell 0.61-m telescope (with diaphragms of 50", corresponding to about 25 000 km at the comet, 100", and 150" aperture) at Cerro Tololo Interamerican Observatory. In this period, we detected an increase in CO+ emission, given by the intensity ratio (CO+ 426 nm)/(continuum 365 nm), of 35 percent in the outer coma, and emission from C2, (C2 514 nm)/(continuum 485 nm), also increased outwards by 80 percent. Emissions from C3 and H2O+ have constant strength over the observed regions." Total visual magnitude estimate by V. F. de Assis Neto, Sao Francisco de Oliveira, Brazil (naked eye): Apr. 27.00 UT, 4.8. G. Garradd, Tamworth, N.S.W., reports a tail disconnection on photographs obtained Apr. 20.8. COMET SORRELLS (1986n) Total visual magnitude estimates: Feb. 18.14 UT, 8.9 (C. S. Morris, Whitaker Peak, CA, 0.26-m reflector); Apr. 23.48, 9.8 (A. Hale, Las Cruces, NM, 0.20-m reflector). 1987 April 27 (4375) Daniel W. E. Green
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