Swift/BAT detects renewed activity from V0332+53

Details Swift/BAT detects renewed activity from V0332+53 Swift/BAT detects renewed activity from V0332+53

Nov 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2319....1k&link_type=abstract

The Astronomer's Telegram, #2319

Astronomy and Astrophysics

Astronomy

2

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

Scientific paper

The Swift/BAT hard X-ray transient monitor reports increased activity in the 15-50 keV band for the transient pulsar and Be/X-ray binary V0332+53. Starting on 2009-11-24 (MJD 55159), the source has increased rapidly in intensity from an undetectable level (one-sigma upper limit of 0.002 cts/cm2/sec or 8 mcrab) up to a current level of 0.012 ± 0.003 cts/cm2/sec (50 mcrab) on 2009-11-29. This is the highest rate seen in the BAT monitor since its outburst in late October 2008 (Krimm et al, ATel #1792).

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