Swift reports a recent brightening of XTE J1543-568

Details Swift reports a recent brightening of XTE J1543-568 Swift reports a recent brightening of XTE J1543-568

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012atel.4008....1k&link_type=abstract

The Astronomer's Telegram, #4008

Astronomy and Astrophysics

Astronomy

X-Ray, Binary, Neutron Star, Transient

Scientific paper

The Swift/BAT hard X-ray transient monitor has recorded a recent flux increase from the transient X-ray pulsar and likely Be binary system XTE J1543-568. In the 15-50 keV band, the source was first detected in an 8-day integration covering 2012 March 9-16 (MJD 55995-56002) with a rate of 0.0016 ± 0.0003 ct/s/cm2. The peak day in the light curve was 2012 March 22 when the rate was 0.0043 ± 0.001 ct/s/cm2 (~20 mCrab).

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