Bibcode
Linares, M.; Bozzo, E.; Altamirano, D.; Degenaar, N.; Wijnands, R.; Soleri, P.; Belloni, T.; Di Salvo, T.; D'Ai, A.; Papitto, A.; Riggio, A.; Burderi, L.
Referencia bibliográfica
The Astronomer's Telegram, #3661
Fecha de publicación:
9
2011
Número de citas
4
Número de citas referidas
1
Descripción
Swift has been monitoring the accreting millisecond pulsar IGR
J17498-2921 since the start of its outburst in 2011 August 12 (ATels
#3551, #3555, #3556). We detected two X-ray bursts on Aug. 18 and 28.
During the first ~12 days the average persistent XRT count rate remained
approximately constant at 3-7 c/s. Around Aug. 24 the source count rate
started to decrease slowly, down to ~1 c/s on Sep. 11.