The fifth outburst of IGRJ11215-5952 observed with Swift/XRT

Details The fifth outburst of IGRJ11215-5952 observed with Swift/XRT The fifth outburst of IGRJ11215-5952 observed with Swift/XRT

Feb 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel..994....1r&link_type=abstract

The Astronomer's Telegram, #994

Astronomy and Astrophysics

Astronomy

6

X-Ray, Request For Observations, Binaries, Transients

Scientific paper

IGR J11215-5952 is the first member of the new class of Supergiant Fast X-ray Transients which displays periodic outbursts, with a recurrence time of 329 days (Sidoli et al. 2006,A&A,450,L9; Smith et al.2006,ATEL #766), likely indicative of the orbital period of the binary system. Based on this periodicity, we are performing a monitoring of the source field with Swift/XRT during the times around the fifth outburst, expected to occur on February 8-10.

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