Basic Functions of the Light Curve Analysis of Eclipsing Variables in the Frequency Domain

Details Basic Functions of the Light Curve Analysis of Eclipsing Variables in the Frequency Domain Basic Functions of the Light Curve Analysis of Eclipsing Variables in the Frequency Domain

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.296..209d&link_type=abstract

Astrophysics and Space Science, Volume 296, Issue 1-4, pp. 209-220

Astronomy and Astrophysics

Astrophysics

Eclipsing Variables, Eclipsing Binaries, Light Curve Analysis, Eclipse Functions, Fourier Analysis

Scientific paper

An analytically tractable method of transforming the problem of light curve analysis of eclipsing binaries from the time domain into the frequency domain was introduced by Kopal (1975, 1979, 1990). This method uses a new general formulation of eclipse functions α, the so-called moments A 2m , and their combinations as g 2m = A 2m+2/(A 2m A 2m+4) functions for the basic spherical model. In this paper, I will review the use of these functions in the light curve analysis of eclipsing binaries.

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