Where Are The Circumbinary Planets of Contact Binaries?

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.abstractTo date no circumbinary planets around a contact binary have been discovered, either by the transit method or from eclipse timing variations, even though such binaries are occasionally known to have wide stellar companions. We thus ask: Where are the circumbinary planets of contact binaries? We have simulated the light curves of contact binaries with possible transiting Jovian circumbinary planets considering the available physical and geometric constraints on the system parameters. It would seem that either circumbinary Jovian planets are not formed at all around contact binaries, possibly due to dynamical effects from the binary or third component stars, or that they are present but their discovery has not been possible so far due to larger distortions than expected in the photometric data or in the times of minimum.
dc.description.sponsorshipSci Org Comm
dc.identifier.endpage399
dc.identifier.isbn978-1-58381-877-0
dc.identifier.isbn978-1-58381-876-3
dc.identifier.issn1050-3390
dc.identifier.startpage395
dc.identifier.urihttps://hdl.handle.net/20.500.12428/28069
dc.identifier.volume496
dc.identifier.wosWOS:000369467900094
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.titleWhere Are The Circumbinary Planets of Contact Binaries?
dc.typeConference Object

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