Swift/XRT Observations Confirm that IGR J17091-3624 is in Outburst

Details Swift/XRT Observations Confirm that IGR J17091-3624 is in Outburst Swift/XRT Observations Confirm that IGR J17091-3624 is in Outburst

Feb 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3148....1k&link_type=abstract

The Astronomer's Telegram, #3148

Astronomy and Astrophysics

Astronomy

4

X-Ray, Binary, Transient

Scientific paper

Swift/XRT carried out a 983-s observation starting at 3 Feb 2011 21:29:03 UTC at a pointing location chosen so that both IGR J17091-3624 and IGR J17098-3628 were in the field of view. IGR J17091-3624 is strongly detected in the XRT image in Photon Counting mode, consistent with the proposed identification of the outburst source from the Swift/BAT data (Krimm et al., ATel #3144). There is no detection of any X-ray flux from IGR J17098-3628.

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