MAXI/GSC detects X-ray rebrightening of the recurrent transient V0332+53

Details MAXI/GSC detects X-ray rebrightening of the recurrent transient V0332+53 MAXI/GSC detects X-ray rebrightening of the recurrent transient V0332+53

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2427....1n&link_type=abstract

The Astronomer's Telegram, #2427

Astronomy and Astrophysics

Astronomy

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

Scientific paper

Following the previous outbursts (Atel #2319, #2369) MAXI/GSC has again detected an X-ray activity of the recurrent transient binary X-ray pulsar V0332+53. These series of 3 outbursts are observed after an interval of 27 years (Stella et al. 1985, ApJ, 288, L45). The one-day averaged flux in the 1.5-20 keV band reached ~20 mCrab on 5 February 2010 (MJD 55232). The current increasing trend of the source flux is comparable to those of the previous activities.

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