Time-resolved Photometry and Spectroscopy of the Cataclysmic Variable V592 Cassiopeiae

Details Time-resolved Photometry and Spectroscopy of the Cataclysmic Variable V592 Cassiopeiae Time-resolved Photometry and Spectroscopy of the Cataclysmic Variable V592 Cassiopeiae

Jul 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998pasp..110..784h&link_type=abstract

The Publications of the Astronomical Society of the Pacific, Volume 110, Issue 749, pp. 784-793.

Astronomy and Astrophysics

Astronomy

19

Stars: Novae, Cataclysmic Variables, Stars: Individual (V592 Cassiopeiae), Stars: Individual (Ls I 55 Deg-8)

Scientific paper

Over the past 10 years, the cataclysmic variable (CV) V592 Cassiopeiae (LS I 55 deg-8) has been monitored by one of the authors. We now present time-resolved optical and infrared photometry and optical spectroscopy of this nova-like binary. Analysis of these data provides the first orbital solution for this star. We find an orbital period near 0.114 days (2.7 hr), a system inclination of 28 deg, and a mass ratio (M_2/M_1) of 0.19. V592 Cas appears to be a nova-like cataclysmic variable with a massive white dwarf primary and lies inside the CV period gap.

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