Solar and stellar rotation

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dc.authoridfiliz ak, nurten/0000-0003-3016-5490
dc.contributor.authorDemircan, O.
dc.contributor.authorEker, Z.
dc.contributor.authorFiliz-Ak, N.
dc.date.accessioned2025-01-27T20:20:38Z
dc.date.available2025-01-27T20:20:38Z
dc.date.issued2007
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.descriptionWorkshop on Solar and Stellar Physics through Eclipses -- MAR 27-29, 2006 -- Ankara Univ, ORSEM Campus, Side, Antalya, TURKEY
dc.description.abstractThe secular evolution of the stellar rotation through angular momentum loss, driven by the stellar wind, and the consequences of the angular momentum transfers between orbit and spinning components in binary star systems will be reviewed with the special emphasis on the Solar rotation. A large co-rotating distance (Alfven radius) of the magnetically driven wind around single stars will be introduced to explain the large angular momentum loss from close binary star systems.
dc.identifier.endpage+
dc.identifier.isbn978-1-583812-38-9
dc.identifier.startpage169
dc.identifier.urihttps://hdl.handle.net/20.500.12428/21772
dc.identifier.volume370
dc.identifier.wosWOS:000246823600022
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.language.isoen
dc.publisherAstronomical Soc Pacific
dc.relation.ispartofSolar and Stellar Physics Through Eclipses
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectChromospherically Active Binaries
dc.subjectOrbital Period Decrease
dc.subjectAngular-Momentum
dc.subjectKinematics
dc.subjectEvolution
dc.subjectStars
dc.titleSolar and stellar rotation
dc.typeConference Object

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