State/Spectral Transition of the Ultraluminous Supersoft X-ray Source in M101

Details State/Spectral Transition of the Ultraluminous Supersoft X-ray Source in M101 State/Spectral Transition of the Ultraluminous Supersoft X-ray Source in M101

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004atel..222....1k&link_type=abstract

The Astronomer's Telegram, #222

Astronomy and Astrophysics

Astronomy

4

X-Ray, Binaries, Black Holes

Scientific paper

We analyzed recent archival Chandra observations of the spiral galaxy, M101, taken between 2004 Jan 19 and 2004 Jan 24. The ultraluminous supersoft X-ray source (CXOU J140332.3+542103) reported by Mukai et al. (2003) and Di Stefano and Kong (2003) was detected in 2 of 3 recent Chandra ACIS-S observations. In the first 56 ksec observation taken on 2004 Jan 19, 27 counts were detected in 0.1-7 keV, with 19 counts below 1.1 keV.

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