Fourier techniques for an analysis of eclipsing binary light curves. IV

Details Fourier techniques for an analysis of eclipsing binary light curves. IV Fourier techniques for an analysis of eclipsing binary light curves. IV

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ap%26ss..62..235d&link_type=abstract

Astrophysics and Space Science, vol. 62, no. 1, May 1979, p. 235-240.

Mathematics

2

Eclipsing Binary Stars, Fourier Transformation, Light Curve, Integral Equations, Least Squares Method, Matrices (Mathematics)

Scientific paper

The aim of the present paper is to establish two further series expansions for the observed light changes of eclipsing binary systems. The coefficients of these expansions have been expressed in the form of general series expansions in terms of the eclipse elements r sub(1, 2), i, and L1 of the spherical model on which all other distorted models may be based in an analysis in the frequency domain.

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