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Circular No. 7840 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Mailstop 18, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. IAUSUBS@CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions) CBAT@CFA.HARVARD.EDU (science) URL http://cfa-www.harvard.edu/iau/cbat.html ISSN 0081-0304 Phone 617-495-7440/7244/7444 (for emergency use only) GAMMA-RAY TRANSIENT S. Golenetskii, R. Aptekar, E. Mazets, and D. Frederiks, Ioffe Institute, St. Petersberg, on behalf of Konus-Wind gamma-ray-burst (GRB) team; T. Cline, Goddard Space Flight Center, NASA, on behalf of the Konus-Wind and Ulysses GRB teams; and K. Hurley, Space Sciences Laboratory, University of California at Berkeley, on behalf of the Ulysses GRB team, report that Konus-Wind and Ulysses observed an exceptional gamma-ray transient from a source with high north-ecliptic latitude of duration > 10 000 s, beginning about Feb. 24.625 UT. Triangulation gives an annulus centered at R.A. = 17h21m46s.3, Decl. = +78o12'29" (equinox 2000.0), with radius 46.138 +/- 1.215 deg. This localization is inconsistent with a solar origin, and the error box excludes all known soft-gamma-ray repeaters (SGR), but it does include Cygnus X-1. In the past seven years, at least two similar transients have been observed by Konus and Ulysses (cf. Mazets et al. 1995, AIP Conf. Proc. 384, 492). Konus-Ulysses triangulation of the two 1995 events gives the following annulus centers and radii: Jan. 10.271-10.368, R.A. = 21h28m32s.4, Decl. = -45o45'32", 82.981 +/- 1.574 deg; Mar. 25.258-25.302, R.A. = 23h15m40s.1, Decl. = +0 56'31", 58.963 +/- 1.782 deg. These localizations are similarly inconsistent with a solar or SGR origin. The three annuli intersect to form an approximately 8-deg**2 error box that includes Cyg X-1. M. Briggs (private comm.) attributed the Mar. 25 event to Cyg X-1. It is concluded that all three outbursts originated from Cyg X-1 while in an exceptionally high state. Fluences (units of 10**-4 erg cm**-2) and peak fluxes (10**-7 erg cm**-2 s**-1) of these events above 15 keV, and corresponding energies (10**41 erg) and luminosities (10**38 erg/s), are: 1995 Jan. 10, 8.4, 2, 6.25, 1.5; Mar. 25, 3.0, 3, 2.2, 2.2; 2002 Feb. 24, 1.5, 1.5, 1.1, 1.1. These fluxes are an order of magnitude higher than fluxes measured by RXTE during a peculiar flaring episode of Cyg X-1 one year ago (Cui et al. 2002, Ap.J. 564, L78). This is the first time that the Interplanetary Network has been used to localize a cosmic transient source that is not an SGR or a GRB. SUPERNOVA 2002bh IN UGC 5286 W. M. Wood-Vasey, University of California at Berkeley and Lawrence Berkeley National Laboratory, reports that pre-discovery CCD images of SN 2002bh (cf. IAUC 7837) taken with the Oschin 1.22-m telescope at Palomar on Feb. 16.4 UT show the new object at unfiltered mag 17.6. (C) Copyright 2002 CBAT 2002 March 4 (7840) Daniel W. E. Green
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