Fourier analysis of the light curves of eclipsing variables. XVI

Details Fourier analysis of the light curves of eclipsing variables. XVI Fourier analysis of the light curves of eclipsing variables. XVI

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ap%26ss..56..453d&link_type=abstract

Astrophysics and Space Science, vol. 56, no. 2, July 1978, p. 453-472.

Mathematics

8

Celestial Mechanics, Eclipsing Binary Stars, Fourier Analysis, Light Curve, Stellar Occultation, Descriptive Geometry, Functions (Mathematics), Limb Darkening, Phase Shift, Stellar Atmospheres

Scientific paper

Different combinations of the 'rectified' eclipse moments A(2m) are used to establish g-functions for the purpose of constituting two independent relations between two unknown parameters. The parameters, which indicate solutions of the elements of the eclipsing system in the frequency-domain, are obtained from the two relations by numerical techniques. The choice of the most suitable moments is considered with attention to the m-dependence of the moments, errors in the observational values of the moments, and different practical procedures for the solution of eclipse elements.

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