Circular No. 5584 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. Telephone 617-495-7244/7440/7444 (for emergency use only) TWX 710-320-6842 ASTROGRAM CAM EASYLINK 62794505 MARSDEN@CFA or GREEN@CFA (.SPAN, .BITNET or .HARVARD.EDU) SUPERNOVA 1992au IN ANONYMOUS GALAXY M. Hamuy, Cerro Tololo Interamerican Observatory; and J. Maza, University of Chile, report the discovery by R. Antezana (University of Chile), on an objective-prism unfiltered IIIa-J plate (90- min) taken by J. Maza and M. Wischnjewsky with the CTIO Curtis Schmidt telescope on July 29.25 UT, of an apparent supernova (mpg about 17) located about 21" east and 9" north of the nucleus of a galaxy at R.A. = 0h08m08s, Decl. = -50 13'.6 (equinox 1950.0). Confirmation was made by R. Aviles (CTIO) on CCD B and V images obtained on Aug. 10.39 with the CTIO 0.9-m telescope. GRO J0422+32 B. A. Harmon, R. B. Wilson, G. J. Fishman, and C. A. Meegan, Marshall Space Flight Center, NASA; W. S. Paciesas and M. S. Briggs, University of Alabama, Huntsville; M. H. Finger, Computer Sciences Corporation; R. Cameron, Universities Space Research Association; and R. Kroeger, and E. Grove, Naval Research Laboratory, report for BATSE and OSSE: "The hard x-ray/gamma-ray transient discovered by the BATSE experiment on the Compton Observatory (IAUC 5580) continued to emit at high intensity, about 3 Crab (40-230 keV), over the past three days. The Observatory was re-pointed on Aug. 11.07 UT, so that the source is observable by all four Compton instruments. An improved location based on combined BATSE and OSSE data is R.A. = 4h22m.1, Decl. = +32 49' (equinox J2000.0; uncertainty radius of 0.2 deg). A significant flux is seen to at least 500 keV, with a hard spectrum. The source continues to show strong variability on all timescales." NOVA CYGNI 1992 C. E. Woodward, and R. A. Hermann, University of Wyoming, report the following infrared magnitudes, obtained using a bolometer on the 2.3-m Wyoming Infrared Observatory telescope on July 28.4 UT: K = 8.21 +/- 0.17, L = 6.94 +/- 0.19, M = 5.87 +/- 0.28, [12.6 microns] = 2.28 +/- 0.33. NOVA SCORPII 1992 Photometry by P. M. Kilmartin, Mt. John University Observatory: Aug. 5.50 UT, V = 8.33 +/- 0.02, B-V = +1.11 +/- 0.01, U-B = +0.21 +/- 0.04, V-R = +0.78 +/- 0.01, V-I = +1.60 +/- 0.02. 1992 August 12 (5584) Daniel W. E. Green
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