Gravitational waves from accreting neutron stars

S. Bonazzola; E. Gourgoulhon

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arXiv · astro-ph/9606123

Gravitational waves from accreting neutron stars

S. Bonazzola·E. Gourgoulhon

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Abstract

We show that accreting neutron stars in binary systems or in Landau-Thorne-Zytkow objects are good candidates for continuous gravitational wave emission. Their gravitational radiation is strong enough to be detected by the next generation of detectors having a typical noise of 10^{-23} Hz^{-1/2}.

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S. Bonazzola, E. Gourgoulhon. 1996-06-20. Gravitational waves from accreting neutron stars. https://arxiv.org/abs/astro-ph/9606123

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