Basic functions of the light curve analysis of eclipsing variables in the frequency domain
dc.contributor.author | Demircan, O | |
dc.date.accessioned | 2025-01-27T20:31:30Z | |
dc.date.available | 2025-01-27T20:31:30Z | |
dc.date.issued | 2005 | |
dc.department | Çanakkale Onsekiz Mart Üniversitesi | |
dc.description | International Conference on Zdenek Kopals Binary Star Legacy -- MAR 31-APR 03, 2004 -- Litomysl, CZECH REPUBLIC | |
dc.description.abstract | 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. | |
dc.identifier.doi | 10.1007/s10509-005-4447-6 | |
dc.identifier.endpage | 220 | |
dc.identifier.issn | 0004-640X | |
dc.identifier.issue | 1-4 | |
dc.identifier.startpage | 209 | |
dc.identifier.uri | https://doi.org/10.1007/s10509-005-4447-6 | |
dc.identifier.uri | https://hdl.handle.net/20.500.12428/23175 | |
dc.identifier.volume | 296 | |
dc.identifier.wos | WOS:000228820000030 | |
dc.identifier.wosquality | Q4 | |
dc.indekslendigikaynak | Web of Science | |
dc.language.iso | en | |
dc.publisher | Springer | |
dc.relation.ispartof | Astrophysics and Space Science | |
dc.relation.publicationcategory | Konferans Öğesi - Uluslararası - Kurum Öğretim Elemanı | |
dc.rights | info:eu-repo/semantics/closedAccess | |
dc.snmz | KA_WoS_20250125 | |
dc.subject | eclipsing variables | |
dc.subject | eclipsing binaries | |
dc.subject | light curve analysis | |
dc.subject | eclipse functions | |
dc.subject | Fourier analysis | |
dc.title | Basic functions of the light curve analysis of eclipsing variables in the frequency domain | |
dc.type | Conference Object |