Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-03-25
Astronomy and Astrophysics
Astrophysics
14 pages including 1 table and 4 figures, Accepted to ApJ Letters
Scientific paper
10.1086/312037
Excellent coverage of the 1998 outburst of the X-ray Nova XTE J1550-564 was provided by the Rossi X-ray Timing Explorer. XTE J1550-564 exhibited an intense (6.8 Crab) flare on 1998 September 19 (UT), making it the brightest new X-ray source observed with RXTE. We present a spectral analysis utilizing 60 Proportional Counter Array spectra from 2.5-20 keV spanning 71 days, and a nearly continuous All Sky Monitor light curve. The spectra were fit to a model including multicolor blackbody disk and power-law components. XTE J1550-564 is observed in the very high, high/soft, and intermediate canonical outburst states of Black Hole X-ray Novae.
Bailyn Charles D.
Levine Alan M.
McClintock Jeff E.
Morgan Edward Harrington
Orosz Jerome A.
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