Further re-brightening of the black hole candidate MAXI J1659-152

Details Further re-brightening of the black hole candidate MAXI J1659-152 Further re-brightening of the black hole candidate MAXI J1659-152

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3379....1y&link_type=abstract

The Astronomer's Telegram, #3379

Astronomy and Astrophysics

Astronomy

1

Optical, Ultra-Violet, X-Ray, Binary, Black Hole, Transient

Scientific paper

Following our previous reports on a sudden drop but later a steep increase of the source intensity of the black hole candidate MAXI J1659-152 (ATels #3298, #3339, see also ATel #3358), we continued to monitor the source with Swift. An observation was carried out on 2011-05-21 13:10:19 UT with an exposure ~2.9 ks. Our new observation shows that the source re-brightening is continuing. The energy spectrum can be well fitted with an absorbed power-law model.

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