Angular Momentum Loss by Magnetic Braking and Gravitational Radiation in Relativistic Binary Stars
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Date
2008
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Proceedings of Science (PoS)
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Abstract
Angular 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.
Description
7th Microquasar Workshop: Microquasars and Beyond, MQW 2008; Foca, Izmir; Turkey; 1 September 2008 through 5 September 2008
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Keywords
Stars, Angular momentum loss, Dynamical evolution, Gravitational radiation, Physical parameters
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Citation
Yakut, 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.
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7th Microquasar Workshop: Microquasars and Beyond, MQW 2008
