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Fourier techniques for an analysis of eclipsing binary light curves: IV
Authors:Osman Demircan
Institution:(1) Dept. of Astronomy, University of Manchester, England;(2) Present address: Dept. of Astronomy, Garyounis University, Benghazi, Libya
Abstract:The aim of the present paper is to establish two further series expansions (alternative to those given in Demircan, 1979a, b, c), for the observed light changes of eclipsing binary system. The coefficients of these expansions have also been expressed in the form of general series expansions in terms of the eclipse elementsr 1.2,i andL 1 of the spherical model on which all other distorted models may be based (Kopal, 1975, 1976) in an analysis in the frequency-domain.
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