INTEGRAL observes further hard X-ray activity of IGR J17586-2129

Details INTEGRAL observes further hard X-ray activity of IGR J17586-2129 INTEGRAL observes further hard X-ray activity of IGR J17586-2129

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2194....1s&link_type=abstract

The Astronomer's Telegram, #2194

Astronomy and Astrophysics

Astronomy

X-Ray, Gamma Ray, Binaries, Black Holes, Neutron Stars, Transients, Variables

Scientific paper

An outburst of IGR J17586-2129 (CXOU J175834.5-212321/Swift J175834.6-212331), a possible highly obscured high-mass X-ray binary (Tomsick et al. 2009, ApJ 701, 811), has been reported using Swift observations. The outburst started by the end of June 2009 and an initial decline was seen in mid- August 2009 (ATel #2156). Since then it has continued to decline to near the Swift/BAT detection limits at the end of August 2009.

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