GRO J1008-57 entering a new outburst at hard X-rays

Details GRO J1008-57 entering a new outburst at hard X-rays GRO J1008-57 entering a new outburst at hard X-rays

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1619....1e&link_type=abstract

The Astronomer's Telegram, #1619

Astronomy and Astrophysics

Astronomy

1

X-Ray, Request For Observations, Binaries, Neutron Stars, Transients

Scientific paper

During the current AGILE pointing at the Vela region, started on 2008 June 30, SuperAGILE detects increasing hard X-ray emission from the Be transient binary pulsar GRO J1008-57, usually below the detection threshold on day-timescale. In the 20-60 keV energy range the source was detected at 30 mCrab level in the 24 hours starting on 2008 July 15 09:00 UT. In the subsequent 24 hours the average flux increased to 45 mCrab, and in the last 24 hours it rose to about 65 mCrab.

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