Please use this identifier to cite or link to this item: https://hdl.handle.net/11147/1948
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dc.contributor.authorYakut, Kadri-
dc.contributor.authorUlaş, Burak-
dc.contributor.authorKalomeni, Belinda-
dc.contributor.authorGülmen, Ömür-
dc.date.accessioned2016-07-21T08:22:34Z
dc.date.available2016-07-21T08:22:34Z
dc.date.issued2005-11
dc.identifier.citationYakut, K., Ulaş, B., Kalomeni, B., and Gülmen, Ö. (2005). Basic physical properties of the low-temperature contact binary system V781 Tau and the near-contact binary system V836 Cyg. Monthly Notices of the Royal Astronomical Society, 363(4), 1272-1278. doi:10.1111/j.1365-2966.2005.09534.xen_US
dc.identifier.issn0035-8711
dc.identifier.issn1365-2966-
dc.identifier.issn0035-8711-
dc.identifier.urihttp://doi.org/10.1111/j.1365-2966.2005.09534.x
dc.identifier.urihttp://hdl.handle.net/11147/1948
dc.description.abstractWe present a detailed photometric study of the low-temperature contact binary V781 Tau, and the near-contact binary V836 Cyg. We have combined the parameters obtained from the light-curve analysis with those found by the spectral studies and we have determined the orbital and physical parameters of the stars. We have collected the times of the mid-eclipses obtained so far and combined with the times obtained in this study. By analysing all these data we determined the mass transfer rate from the massive star to the less massive one for V781 Tau, and from the less massive component to the massive one in the case of V836 Cyg. Finally, we have compared the results obtained for V781 Tau and for V836 Cyg with similar systems.en_US
dc.description.sponsorshipTÜBİTAKen_US
dc.language.isoenen_US
dc.publisherOxford University Pressen_US
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectBinariesen_US
dc.subjectEclipsingen_US
dc.subjectFundamental parametersen_US
dc.subjectStarsen_US
dc.subjectV836 Cygen_US
dc.subjectV781 Tauen_US
dc.titleBasic physical properties of the low-temperature contact binary system V781 Tau and the near-contact binary system V836 Cygen_US
dc.typeArticleen_US
dc.authoridTR17457en_US
dc.institutionauthorKalomeni, Belinda-
dc.departmentİzmir Institute of Technology. Physicsen_US
dc.identifier.volume363en_US
dc.identifier.issue4en_US
dc.identifier.startpage1272en_US
dc.identifier.endpage1278en_US
dc.identifier.wosWOS:000232867000019en_US
dc.identifier.scopus2-s2.0-27744451889en_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.identifier.doi10.1111/j.1365-2966.2005.09534.x-
dc.relation.doi10.1111/j.1365-2966.2005.09534.xen_US
dc.coverage.doi10.1111/j.1365-2966.2005.09534.xen_US
dc.identifier.wosqualityQ1-
dc.identifier.scopusqualityQ1-
item.openairetypeArticle-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
item.languageiso639-1en-
item.cerifentitytypePublications-
item.grantfulltextopen-
Appears in Collections:Physics / Fizik
Scopus İndeksli Yayınlar Koleksiyonu / Scopus Indexed Publications Collection
WoS İndeksli Yayınlar Koleksiyonu / WoS Indexed Publications Collection
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