Angular Momentum Loss and Gravitational wave amplitudes for X-ray   Binaries with a Neutron Star Component
  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. 
T. \.I\c{c}li and K. Yakut
astro-ph.SR astro-ph.HE