Recent light maximum of BQ Cam

Details Recent light maximum of BQ Cam Recent light maximum of BQ Cam

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2381....1g&link_type=abstract

The Astronomer's Telegram, #2381

Astronomy and Astrophysics

Astronomy

Optical, Binaries, Neutron Stars, Pulsars, Transients, Variables, Stars

Scientific paper

BQ Cam is a binary system consisting of a variable Be type star and a neutron star. It is an optical counterpart of the transient X-ray pulsar V0332+53. The star varies in the ranges between 15.2 and 15.9 mag in the V band, and X-ray outbursts are associated with the maxima of optical brightness. The exclusion was the previous X-ray outburst occurred in 2008 October (MJD 54756) (ATEL#1792) when the brightness was rising to the recent optical maximum at the level of V=15.35, not in the light maximum.

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