Gravitational waves from accreting neutron stars

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dc.creatorBonazzola, S.
dc.creatorGourgoulhon, E.
dc.date1996-06-20
dc.date.accessioned2026-07-07T02:21:24Z
dc.date.available2026-07-07T02:21:24Z
dc.descriptionWe 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}.
dc.description10 pages, no figure, to appear in the Proceedings of the International Conference on Gravitational Waves: Sources and Detectors, Cascina (Pisa), Italy --- March 19-23, 1996, eds. I. Ciufolini, F. Fidecaro (World Scientific, in press)
dc.identifierhttps://arxiv.org/abs/astro-ph/9606123
dc.identifierhttp://arxiv.org/abs/astro-ph/9606123
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10535
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGravitational waves from accreting neutron stars
dc.typetext

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