Relativistic models of kHz QPOs

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dc.creatorKluzniak, W.
dc.date2000-12-29
dc.date.accessioned2026-07-07T01:57:13Z
dc.date.available2026-07-07T01:57:13Z
dc.descriptionAfter reviewing the general-relativistic ``gap'' model of accretion, I discuss its relation to the high frequency quasi-periodic oscillations observed in low-mass X-ray binaries. The ``300'' Hz frequency seen in some X-ray bursts may be a relativistic signature of keplerian rotation of the neutron star.
dc.descriptionto appear in Proc. of the NATO ASI in Elounda, May 1999 "The Black-hole neutron-star connection"
dc.identifierhttps://arxiv.org/abs/astro-ph/0012544
dc.identifierhttp://arxiv.org/abs/astro-ph/0012544
dc.identifierC. Kouveliotou et al., eds., The Neutron Star - Black Hole Connection, (2001), (Kluwer: Dordrecht), 325-330
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2299
dc.subjectAstrophysics
dc.titleRelativistic models of kHz QPOs
dc.typetext

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