End of outburst of IGR J11215-5952; possible pulsations

Details End of outburst of IGR J11215-5952; possible pulsations End of outburst of IGR J11215-5952; possible pulsations

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..773....1s&link_type=abstract

The Astronomer's Telegram, #773

Astronomy and Astrophysics

Astronomy

9

X-Ray, Binaries, Pulsars, Transients

Scientific paper

The recent outburst of IGR J11215-5952, predicted by the ephemeris of Sidoli et al. (2006, astro-ph/0603081) and observed with the Rossi X- ray Timing Explorer (RXTE) (Smith, Bezayiff and Negueruela 2006, ATEL #766) has apparently ended. The first and last observations that showed significant activity began and ended on 22:09UT March 16 and 21:48UT March 18, respectively. Each observation lasted about 1000 s, and three per day were taken from March 15 through March 18.

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