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

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dc.contributor.authorDemircan, O
dc.date.accessioned2025-01-27T20:31:30Z
dc.date.available2025-01-27T20:31:30Z
dc.date.issued2005
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.descriptionInternational Conference on Zdenek Kopals Binary Star Legacy -- MAR 31-APR 03, 2004 -- Litomysl, CZECH REPUBLIC
dc.description.abstractAn 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.
dc.identifier.doi10.1007/s10509-005-4447-6
dc.identifier.endpage220
dc.identifier.issn0004-640X
dc.identifier.issue1-4
dc.identifier.startpage209
dc.identifier.urihttps://doi.org/10.1007/s10509-005-4447-6
dc.identifier.urihttps://hdl.handle.net/20.500.12428/23175
dc.identifier.volume296
dc.identifier.wosWOS:000228820000030
dc.identifier.wosqualityQ4
dc.indekslendigikaynakWeb of Science
dc.language.isoen
dc.publisherSpringer
dc.relation.ispartofAstrophysics and Space Science
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjecteclipsing variables
dc.subjecteclipsing binaries
dc.subjectlight curve analysis
dc.subjecteclipse functions
dc.subjectFourier analysis
dc.titleBasic functions of the light curve analysis of eclipsing variables in the frequency domain
dc.typeConference Object

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