An interpretation of CB light curve of active cataclysmic variable OY Car by using the inverse-problem method.

Details An interpretation of CB light curve of active cataclysmic variable OY Car by using the inverse-problem method. An interpretation of CB light curve of active cataclysmic variable OY Car by using the inverse-problem method.

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995pobeo..49..145d&link_type=abstract

Publications de l'Observatoire Astronomique de Beograd, No. 49, p. 145 - 150

Astronomy and Astrophysics

Astronomy

Cataclysmic Binaries: Light Curves, Dwarf Novae: Models, Dwarf Novae: Accretion Disks

Scientific paper

In the paper a model synthesizing the light curves of novae and novae-like stars, as well as of active close binaries (CB) in the phase of an intensive matter exchange between the components with accretion onto a white dwarf is considered. The model considers the radial and azimuthal temperature distributions in the disc allowing a successful interpretation of asymmetric deformed light curves characteristic of these systems. The analysis of the observed light curves is performed by using the inverse-problem method (Djurašević, 1992) adapted to this model. In the particular case the parameters of the dwarf nova OY Car are estimated on the basis of observations (Wood et al., 1989).

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