MAXI/GSC detects an outburst from a Be/X-ray binary GRO J1008-57

Details MAXI/GSC detects an outburst from a Be/X-ray binary GRO J1008-57 MAXI/GSC detects an outburst from a Be/X-ray binary GRO J1008-57

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2769....1s&link_type=abstract

The Astronomer's Telegram, #2769

Astronomy and Astrophysics

Astronomy

X-Ray, Binaries, Neutron Stars, Pulsars, Transients

Scientific paper

An increase of X-ray flux of the Be/X-ray binary pulsar GRO J1008-57 was observed with MAXI/GSC on 2010 August 1 at 30+-4 mCrab (4-10 keV). This is consistent with the recurrent outburst from this source with a 248-day period since the last one in November 2009 (ATel #2313). The latest light curve and the image of this source are available at the following URL: http://maxi.riken.jp/top/index.php?cid=1&jname=J1009-582 .

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