Bibcode
Linares, M.; Chakrabarty, D.; Cummings, J. R.; Kennea, J. A.; Krimm, H. A.; Markwardt, C. B.
Referencia bibliográfica
The Astronomer's Telegram, #3632
Fecha de publicación:
9
2011
Número de citas
3
Número de citas referidas
2
Descripción
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.