Cataclysmic variables as sources of gravitational waves

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dc.creatorMeliani, M. T.
dc.creatorde Araujo, J. C. N.
dc.creatorAguiar, O. D.
dc.date2000-04-28
dc.date.accessioned2026-07-07T01:53:18Z
dc.date.available2026-07-07T01:53:18Z
dc.descriptionGeneral Relativity predicts that binary systems of stars produce gravitational waves of significant intensity. Here we are particularly interested in the cataclysmic variable binaries (CVs). These systems emit low frequency gravitational waves, $ f < 10^{-3} Hz$. We present here a catalog of CVs and argue that part of them are capable of being detected by the Laser Interferometer Space Antenna (LISA).
dc.description10 pages, 2 eps figures, (A&A) Latex. A&A (in press)
dc.identifierhttps://arxiv.org/abs/astro-ph/0004406
dc.identifierhttp://arxiv.org/abs/astro-ph/0004406
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/918
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCataclysmic variables as sources of gravitational waves
dc.typetext

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