Basic functions of the light curve analysis of eclipsing variables in the frequency domain
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Tarih
2005
Yazarlar
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
