A model of the early type binary system BF Aurigae

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dc.contributor.authorDemircan, O
dc.contributor.authorOzdemir, S
dc.contributor.authorAlbayrak, B
dc.contributor.authorAk, H
dc.contributor.authorTanriver, M
dc.contributor.authorDegirmenci, OL
dc.contributor.authorErdem, A
dc.contributor.authorSezer, C
dc.date.accessioned2019-10-27T11:53:16Z
dc.date.available2019-10-27T11:53:16Z
dc.date.issued1997
dc.departmentEge Üniversitesien_US
dc.description.abstractA physically consistent model is presented for the early-type eclipsing binary system BF Aur, based on a simultaneous solution of its light and radial velocity curves. The less massive fainter (but hotter) secondary is smaller but almost Roche lobe filling component. The system is thus not reverse-algol. The absolute parameters of the system are found to be: M-h = 3.3 M., M-c = 4.1 M., T-h = 15600 K, T-c = 15400 K, R-h = 3.9 R., R-c = 4.1 R.. More accurate radial velocity data are needed before uniqueness can be claimed for the model.en_US
dc.identifier.endpage135en_US
dc.identifier.issn0185-1101
dc.identifier.issn0185-1101en_US
dc.identifier.issue2en_US
dc.identifier.scopusqualityQ3en_US
dc.identifier.startpage131en_US
dc.identifier.urihttps://hdl.handle.net/11454/34870
dc.identifier.volume33en_US
dc.identifier.wosWOS:A1997YF44300008en_US
dc.identifier.wosqualityQ2en_US
dc.indekslendigikaynakWeb of Scienceen_US
dc.indekslendigikaynakScopusen_US
dc.language.isoenen_US
dc.publisherUniv Nacional Autonoma Mexico, Inst De Astronomiaen_US
dc.relation.ispartofRevista Mexicana De Astronomia Y Astrofisicaen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.subjectbinaries-eclipsingen_US
dc.subjectbinaries-spectroscopicen_US
dc.subjectstars-fundamental parametersen_US
dc.subjectstars-individual (BF Aur)en_US
dc.titleA model of the early type binary system BF Aurigaeen_US
dc.typeArticleen_US

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