Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ap%26ss..47...79n&link_type=abstract
Astrophysics and Space Science, vol. 47, Mar. 1977, p. 79-97. Research supported by the Ministry of Coordination and Planning of
Astronomy and Astrophysics
Astrophysics
8
Eclipsing Binary Stars, Light Curve, Finite Element Method, Limb Darkening, Stellar Luminosity, Stellar Magnitude, Stellar Models, Stellar Occultation, Variable Stars
Scientific paper
The aim of the present paper has been to analyse the light changes of the close eclipsing system AK Herculis in the frequency domain. This analysis is based on Kopal's new theory recently developed for the study of light variations - between minima as well as within eclipses - of close eclipsing binaries whose components are distorted by axial rotation and mutual tidal action. A new method for the separation of the photometric proximity and eclipse effects directly from the observed data is also presented. In this method no `rectification' is needed. New elements taking into account the photometric perturbations are also given
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