Angular Momentum Loss by Magnetic Braking and Gravitational Radiation in Relativistic Binary Stars
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Date
2008
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Incoma Ltd
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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. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial- ShareAlike Licence.
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International Conference Recent Advances in Natural Language Processing, RANLP -- 7th Microquasar Workshop: Microquasars and Beyond, MQW 2008 -- 1 September 2008 through 5 September 2008 -- Foca, Izmir -- 101447
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checked on Apr 27, 2026
