Unsubscribe vsnet-alert@00ruri.kusastro.kyoto-u.ac.jp phillips@vzpacifica.net ----- Original Message ----- From: "Ryoko Ishioka" <ishioka@kusastro.kyoto-u.ac.jp> To: <vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp> Sent: Thursday, April 18, 2002 5:37 AM Subject: [vsnet-alert 7299] (Fwd) a new, fast X-ray transient > > Date: Wed, 17 Apr 2002 14:36:22 -0400 (EDT) > From: Ron Remillard <rr@space.mit.edu> > Subject: [vsnet-alert 0] a new, fast X-ray transient > > XTE J1901+014: a new, fast X-ray transient > > The RXTE All-Sky Monitor has discovered a fast X-ray transient that > was initially thought to be a gamma ray burst, reported on the GCN > network as GRB020406. The event began on 2002 April 6.76268, lasting > more than 2 min and less than 3.15 hr, with a peak flux of 0.9 Crab > (2-12 keV). (see http://xte.mit.edu/xtej1901+104). The ASM data show > rapid evolution to a very hard spectrum during this outburst, but the > IPN instruments failed to detect the source above 15 keV (K. Hurley, > private communication). Furthermore, archival ASM data show a previous > outburst at the same position on 1997 June 21.215, which was longer > than 6 min and less than 8 hr, with a peak flux of 0.4 Crab. The > combined ASM observations yield a best position: R.A. = 19h01m36s, > Decl. = +1 26'.4 (equinox J2000.0; estimated 3' uncertainty in > R.A. and 2' uncertainty in Decl.). The error box contains one very > faint, unidentified X-ray source from the Einstein Galactic Plane > Survey: 2E1859.1+0122 (J2000 R.A. = 19h01m40.2s, Decl. = +1 27' 13''; > error radius 48''; Hertz and Grindlay 1988, AJ, 96, 233). The time > scale for these eruptions are reminiscent of the microquasar and black > hole binary V4641 Sgr, so we strongly encourage optical and radio > observations of XTE J1901+014. > > R. A. Remillard (M.I.T.) and D. A. Smith (U. Michigan), for > the RXTE ASM Team at M.I.T. and NASA Goddard Space Flight Center. > > --------------------- > end