RXTE observes further brightening of 4U 1630-47

Details RXTE observes further brightening of 4U 1630-47 RXTE observes further brightening of 4U 1630-47

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2365....1t&link_type=abstract

The Astronomer's Telegram, #2365

Astronomy and Astrophysics

Astronomy

1

X-Ray, Black Holes, Transients

Scientific paper

Observations of 4U 1630-47 were made with the Rossi X-ray Timing Explorer (RXTE), following a report that this black hole transient is now in outburst (Tomida et al., ATEL#2363). The RXTE 3-25 keV spectrum from 2010 Jan. 1 is well-described by a model consisting of a disk-blackbody plus power- law model with absorption. The disk-blackbody temperature is Tin = 1.19 +/- 0.01 keV, and this component dominates below 7 keV.

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