Swift detects an X-ray burst and renewed activity from KS 1741-293

Linares, M.; Chakrabarty, D.; Cummings, J. R.; Kennea, J. A.; Krimm, H. A.; Markwardt, C. B.
Bibliographical reference

The Astronomer's Telegram, #3632

Advertised on:
9
2011
Number of authors
6
IAC number of authors
0
Citations
3
Refereed citations
2
Description
An X-ray burst from the direction of the neutron star (NS) transient and thermonuclear burster KS 1741-293 triggered the Swift-BAT on 2011-09-01 at 12:07:22 UTC. The burst was detected only in the 15-25 keV band, lasted for about 10s, had a peak flux of (9.0+/-2.5)e-9 ergs/cm^2/s and an integrated fluence of (5.5+/-1.2)e-8 erg/cm^2 (both in the 15-150 keV band). The average BAT spectrum can be fitted with a 2.2+/-0.6 keV blackbody model.