Swift detects MAXI J1543-564 transition into hard state

Details Swift detects MAXI J1543-564 transition into hard state Swift detects MAXI J1543-564 transition into hard state

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3662....1k&link_type=abstract

The Astronomer's Telegram, #3662

Astronomy and Astrophysics

Astronomy

1

X-Ray, Transient

Scientific paper

Swift/XRT has been performing regular monitoring observations of the black-hole candidate binary system MAXI J1543-564 (Negoro et al., ATEL #3330) since May 8th, 2010 (Kennea et al., ATEL #3331). The source was seen to go into the soft state, where the spectrum is dominated by thermal emission from the disk, around May 15th, 2011 (e.g. Kennea et al., ATEL #3362, Munoz-Darias et al., ATEL #3355).

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