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Title:
Time-resolved Photometry and Spectroscopy of the Cataclysmic Variable V592 Cassiopeiae
Authors:
Huber, Mark E.; Howell, Steve B.; Ciardi, David R.; Fried, Robert
Affiliation:
AA(Department of Physics and Astronomy, University of Wyoming, Laramie, WY 82071; , , ), AB(Department of Physics and Astronomy, University of Wyoming, Laramie, WY 82071; , , ), AC(Department of Physics and Astronomy, University of Wyoming, Laramie, WY 82071; , , ), AD(Braeside Observatory, P. O. Box 906, Flagstaff, AZ 86002; )
Publication:
The Publications of the Astronomical Society of the Pacific, Volume 110, Issue 749, pp. 784-793. (PASP Homepage)
Publication Date:
07/1998
Origin:
PASP
PASP Keywords:
STARS: NOVAE, CATACLYSMIC VARIABLES, STARS: INDIVIDUAL (V592 CASSIOPEIAE), STARS: INDIVIDUAL (LS I 55 DEG-8)
DOI:
10.1086/316192
Bibliographic Code:
1998PASP..110..784H

Abstract

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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