Continued X-ray Brightening of V0332+53

Details Continued X-ray Brightening of V0332+53 Continued X-ray Brightening of V0332+53

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004atel..371....1r&link_type=abstract

The Astronomer's Telegram, #371

Astronomy and Astrophysics

Astronomy

11

X-Ray, Pulsars, Transients

Scientific paper

The XTE All-Sky monitor shows continued brightening of V0332+53, with an average flux of 1.1 Crab (2-12 keV) during the first half of 2004 Dec. 22. The true flux is certain to be substantially higher since the source is extremely hard, even for X-ray pulsars. The ASM count rate is evaluated here using cameras 2 and 3 only, since detector gain differences for camera 1 skew the results, given that normalizations are tied to the spectrum of the Crab Nebula.

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