BH Lyn: UBVRI and CCD photometry of the eclipsing cataclysmic variable

Details BH Lyn: UBVRI and CCD photometry of the eclipsing cataclysmic variable BH Lyn: UBVRI and CCD photometry of the eclipsing cataclysmic variable

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001oap....14...15a&link_type=abstract

Odessa Astronomical Publications, 14, 15-16

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Stars: Variable: Cataclysmic: Bh Lyn

Scientific paper

We report preliminary results of the UBVRI photoelectric and R CCD observations obtained in the Crimean astrophysical observatory and the Astronomical observatory of the Athens University. The light curve represents well-pronounced eclipses with a total duration of the most sharp phase of 0.022deg. At the eclipse, the color index U--B becomes smaller by 0.2m than outside eclipse, contrary to other colors, where the color indices become larger. This indicates a presence of uneclipsed source of ultraviolet emission, possibly the wind from the accretion disc.

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