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dc.contributor.authorYakut, Kadri
dc.contributor.authorKalomeni, Belinda
dc.contributor.authorTout, C. A.
dc.date.accessioned2016-10-21T08:56:57Z
dc.date.available2016-10-21T08:56:57Z
dc.date.issued2008
dc.identifier.citationYakut, K., Kalomeni, B., and Tout, C. A. (2008, September 1-5). Angular momentum loss by magnetic braking and gravitational radiation in relativistic binary stars. Paper presented at the 7th Microquasar Workshop: Microquasars and Beyond, MQW 2008, Foça, İzmir; Turkey.en_US
dc.identifier.urihttp://hdl.handle.net/11147/2301
dc.description7th Microquasar Workshop: Microquasars and Beyond, MQW 2008; Foca, Izmir; Turkey; 1 September 2008 through 5 September 2008en_US
dc.description.abstractAngular momentum loss (AML) mechanisms and dynamical evolution owing to magnetic braking and gravitational radiation in relativistic binary stars (RBS) are studied with use of physical parameters collected from the literature. We have calculated and compared AML time scales for the RBS with non-degenerate components and double degenerate (DD) systems.en_US
dc.description.sponsorshipTurkish Scientific and Technical Research Councilen_US
dc.language.isoengen_US
dc.publisherInternational Conference Recent Advances in Natural Language Processing, RANLPen_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectStarsen_US
dc.subjectAngular momentum lossen_US
dc.subjectDynamical evolutionen_US
dc.subjectGravitational radiationen_US
dc.subjectPhysical parametersen_US
dc.titleAngular momentum loss by magnetic braking and gravitational radiation in relativistic binary starsen_US
dc.typeconferenceObjecten_US
dc.contributor.authorIDTR17457en_US
dc.contributor.iztechauthorKalomeni, Belinda
dc.relation.journal7th Microquasar Workshop: Microquasars and Beyond, MQW 2008en_US
dc.contributor.departmentIzmir Institute of Technology. Physicsen_US
dc.identifier.scopusSCOPUS:2-s2.0-84890659569
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanıen_US


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