The black hole candidate IGR J17091-3624 is still active

Details The black hole candidate IGR J17091-3624 is still active The black hole candidate IGR J17091-3624 is still active

Feb 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012atel.3913....1a&link_type=abstract

The Astronomer's Telegram, #3913

Astronomy and Astrophysics

Astronomy

1

X-Ray, Binary, Black Hole, Transient

Scientific paper

In February 2011 it was reported that the black hole candidate IGR J17091--3624 exhibited a new outburst (using Swift/BAT, see Atel #3144). During this outburst IGR J17091-3624 was followed up by multi-wavelength observations (ATel #3148, #3150, #3159, #3167, #3168, #3179, #3203, #3225, #3229, #3230, #3232, #3266, #3299). After IGR J17091-3624 underwent the typical hard-to-soft state transition (e.g.

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