Differential correction for SPOT parameters in the RS CVn system RT Coronae Borealis

Details Differential correction for SPOT parameters in the RS CVn system RT Coronae Borealis Differential correction for SPOT parameters in the RS CVn system RT Coronae Borealis

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989cha%26a..13....9z&link_type=abstract

Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 13, March 1989, p. 9-17. Translation.

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3

Astronomical Photometry, Computational Astrophysics, Eclipsing Binary Stars, Irregular Variable Stars, Light Curve, Starspots, Chromosphere, Ubv Spectra

Scientific paper

The 1983 edition of the Wilson-Devinney program is extended by including differential correction for spot parameters. A grid method is proposed for determining the spot latitude. Applying this to the outside eclipse distortion wave in the RS CVn type eclipsing binary RT CrB, the positions, sizes, and temperatures of two spots on the secondary component and a theoretical light curve that reproduced well the observed features of the distortion wave are obtained.

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