Light curves of the eclipsing systems of RS CVn-type

Details Light curves of the eclipsing systems of RS CVn-type Light curves of the eclipsing systems of RS CVn-type

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.162..205b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 162, no. 2, Dec. 1989, p. 205-209. Research supported by Universidad de La

Astronomy and Astrophysics

Astronomy

2

Astronomical Photometry, Eclipsing Binary Stars, Light Curve, Limb Darkening, Stellar Rotation, Stellar Systems, Axes Of Rotation, Line Of Sight, Radio Sources (Astronomy), X Ray Sources

Scientific paper

The light curves for rotating spotted stars generated by a computational code developed in this work are presented. This code is based in a model of the system and its analytical solution. The paper also presents an analysis of the photometric curve variations with the changes in the model's parameters. As a first result, a temporal evolution of the light curve when the photospheric spot varies its size and position is simulated, and some observational light curves of the II Peg star are reproduced.

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