Nature of the Multiple System V831 Centauri

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dc.authoridBAKIS, VOLKAN/0000-0002-3125-9010
dc.contributor.authorBakis, V.
dc.contributor.authorHensberge, H.
dc.contributor.authorDemircan, O.
dc.date.accessioned2025-01-27T21:07:36Z
dc.date.available2025-01-27T21:07:36Z
dc.date.issued2010
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.descriptionInternational Conference on Binaries - Key to the Comprehension of the Universe -- JUN 08-12, 2009 -- Masaryk Univ, Dept Theoret Phys & Astrophys, Brno, CZECH REPUBLIC
dc.description.abstractWe present a comprehensive analysis results of the high-resolution spectra together with photometric data of the multiple system V831 Centaurus. Using spectral disentangling technique on the spectroscopic data with information from multi-band Geneva photometry, the disentangled spectra of the close binary components and the third star were obtained together with the spectroscopic orbital elements. The mass ratio of the close binary was found to be q=0.805. The disentangled spectra of the close binary components present a characteristic behavior of mid-B spectral type star while the third star's spectrum is more consistent with a mid-F spectral type main-sequence star.
dc.identifier.endpage+
dc.identifier.isbn978-1-58381-750-6
dc.identifier.startpage109
dc.identifier.urihttps://hdl.handle.net/20.500.12428/28117
dc.identifier.volume435
dc.identifier.wosWOS:000289880000030
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.language.isoen
dc.publisherAstronomical Soc Pacific
dc.relation.ispartofBinaries - Key To Comprehension of The Universe
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.titleNature of the Multiple System V831 Centauri
dc.typeConference Object

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