Circumbinary Components of Contact Binaries

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dc.contributor.authorDemircan, Osman
dc.contributor.authorBulut, Ibrahim
dc.date.accessioned2025-01-27T21:07:28Z
dc.date.available2025-01-27T21:07:28Z
dc.date.issued2015
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.descriptionConference on Living Together: Planets, Host Stars and Binaries -- SEP 08-12, 2014 -- Litomysl, CZECH REPUBLIC
dc.description.abstractPeriod changes in contact binaries obtained by the analysis of times of eclipse are often found to be chaotic in nature. However, they may be representable by a few cyclic changes superposed on a secular change. The cyclic changes are most likely caused by third components revolving around the contact binaries. This contribution shows some typical examples of the period changes in contact binaries.
dc.description.sponsorshipSci Org Comm
dc.identifier.endpage117
dc.identifier.isbn978-1-58381-877-0
dc.identifier.isbn978-1-58381-876-3
dc.identifier.startpage114
dc.identifier.urihttps://hdl.handle.net/20.500.12428/28068
dc.identifier.volume496
dc.identifier.wosWOS:000369467900017
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.language.isoen
dc.publisherAstronomical Soc Pacific
dc.relation.ispartofLiving Together: Planets, Host Stars, and Binaries
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.titleCircumbinary Components of Contact Binaries
dc.typeConference Object

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