T. İçli, K. Yakut
Published 2016-03-12Version 1
Binary systems with neutron stars and double degenerate systems are crucial objects to test current stellar evolution models and Einstein's general relativity. In this study, we present angular momentum loss mechanism via gravitational radiation and magnetized stellar winds for some selected systems with a neutron star. We calculated and plotted their time scales for angular momentum loss. Gravitational wave amplitudes of binary systems with a neutron star components are also estimated and their detectability with a gravitational wave detector (LISA) has been plotted.
Comments: 4 pages, 3 figures. Proceedings 28th Texas Symposium on Relativistic Astrophysics, Geneva (Switzerland), 13-18 December 2015
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Mass and angular momentum loss via decretion disks
The dependence of stellar mass and angular momentum losses on latitude and on active region and dipolar magnetic fields
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