Angular momentum loss by magnetic braking and gravitational radiation in relativistic binary stars

Please use this identifier to cite or link to this item: https://hdl.handle.net/11147/2301

Title:	Angular momentum loss by magnetic braking and gravitational radiation in relativistic binary stars
Authors:	Yakut, Kadri Kalomeni, Belinda Tout, C. A.
Keywords:	Stars Angular momentum loss Dynamical evolution Gravitational radiation Physical parameters
Publisher:	Proceedings of Science (PoS)
Source:	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.
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
URI:	http://hdl.handle.net/11147/2301
Appears in Collections:	Physics / Fizik Scopus İndeksli Yayınlar Koleksiyonu / Scopus Indexed Publications Collection