Optical Brightening of Be/X-ray Binary BQ Cam/V0332+53.

Details Optical Brightening of Be/X-ray Binary BQ Cam/V0332+53. Optical Brightening of Be/X-ray Binary BQ Cam/V0332+53.

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004atel..245....1g&link_type=abstract

The Astronomer's Telegram, #245

Astronomy and Astrophysics

Astronomy

13

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

Scientific paper

BQ Cam is an optical counterpart of X-ray transient V0332+53. The system consists of a Be star and a neutron star. Recently, it has undergone rapid brightening after 9.3 years of quiescence, and has reached its brightness maximum V=15.19 on 2004 January 31. Our photometric CCD monitoring made with SAI 60-cm and SAO 100-cm reflectors shows that the continuous rise to maximum began in January, 2002 at V=15.66.

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