Basic functions of the light curve analysis of eclipsing variables in the frequency domain

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Tarih

2005

Dergi Başlığı

Dergi ISSN

Cilt Başlığı

Yayıncı

Springer

Erişim Hakkı

info:eu-repo/semantics/closedAccess

Özet

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 alpha, 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.

Açıklama

International Conference on Zdenek Kopals Binary Star Legacy -- MAR 31-APR 03, 2004 -- Litomysl, CZECH REPUBLIC

Anahtar Kelimeler

eclipsing variables, eclipsing binaries, light curve analysis, eclipse functions, Fourier analysis

Kaynak

Astrophysics and Space Science

WoS Q Değeri

Q4

Scopus Q Değeri

Cilt

296

Sayı

1-4

Künye