Swift XRT and UVOT observations of renewed activity from MAXI J1836-194

Details Swift XRT and UVOT observations of renewed activity from MAXI J1836-194 Swift XRT and UVOT observations of renewed activity from MAXI J1836-194

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012atel.3975....1y&link_type=abstract

The Astronomer's Telegram, #3975

Astronomy and Astrophysics

Astronomy

X-Ray, Transient

Scientific paper

We report a pointed Swift observation of the black hole X-ray transient MAXI J1836-194 (ATel #3611, #3613). The source is suggested to be a black hole candidate based on its timing and spectral properties, and the radio detection during the rise of the previous outburst (ATels #3618, #3628). The source was first detected by MAXI/GSC on August 30, 2011 (ATel #3611), and it was on for about 3 months.

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