Angular Momentum Loss by Magnetic Braking and Gravitational Radiation in Relativistic Binary Stars

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dc.creatorYakut, K.
dc.creatorKalomeni, B.
dc.creatorTout, C. A.
dc.date2008-11-04
dc.date.accessioned2026-07-07T10:15:22Z
dc.date.available2026-07-07T10:15:22Z
dc.descriptionAngular 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.
dc.description6 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/0811.0455
dc.identifierhttp://arxiv.org/abs/0811.0455
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/173153
dc.subjectAstrophysics
dc.titleAngular Momentum Loss by Magnetic Braking and Gravitational Radiation in Relativistic Binary Stars
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