出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：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.
