Direct photometric problem for spotted stars

Details Direct photometric problem for spotted stars Direct photometric problem for spotted stars

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.136..289k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 136, no. 2, Aug. 1987, p. 289-297.

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Astronomical Photometry, Eclipsing Binary Stars, Starspots, Computational Astrophysics, Variability

Scientific paper

In the framework of the direct photometric problem the author obtained an analytical representation of the light variations of binary systems of stars, one of which having spots on its surface. The photometric effect is due to the mutual eclipses and to the rotation of the spotted component. These expressions can be used for the solution of the inverse problem for spotted stars.

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