H1743-322 back to the quiescence

Details H1743-322 back to the quiescence H1743-322 back to the quiescence

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1414....1c&link_type=abstract

The Astronomer's Telegram, #1414

Astronomy and Astrophysics

Astronomy

2

X-Ray, Binaries, Black Holes, Transients

Scientific paper

We followed the BHC H1743-322/IGR J17464-3213 (ATels #1348,#1349,#1352) with Swift/XRT during the decreasing phase of the outburst until quiescence for a total amount of 20 ks (in 6 pointings). The observations were performed two times per week from 2008 February 12th at 01:31:00 UT until March 5 13:19:18 UT. The source flux decreasing along the observing period occurred with a constant spectral shape, namely an absorbed power-law.

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