INTEGRAL observations of GRO J1008-57 in outburst

Details INTEGRAL observations of GRO J1008-57 in outburst INTEGRAL observations of GRO J1008-57 in outburst

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.1995....1l&link_type=abstract

The Astronomer's Telegram, #1995

Astronomy and Astrophysics

Astronomy

1

X-Ray, Gamma Ray, Binaries, Pulsars, Transients

Scientific paper

The Be X-ray binary GRO J1008-57 is known to display regular outburts, with a period of 248 days (ATel #940; Coe et al. 2007, MNRAS 378, 1427). In the past, it has been detected by INTEGRAL at a level of 30 mCrab in October 2005 (ATel #647; in the 18-45 keV energy range), but also in June 2004 (Coe et al. 2007). Swift/BAT detected a brighter than usual flare in November 2007 (ATel #1298), with a level of 100 mCrab up to 400 mCrab (in the 15-50 keV energy range; see >the Swift/BAT lightcurve).

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