Epicyclic Frequencies and Resonant Phenomena Near Black Holes: The Current Status

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dc.creatorAliev, Alikram N.
dc.date2006-12-27
dc.date2007-01-03
dc.date.accessioned2026-07-07T07:37:47Z
dc.date.available2026-07-07T07:37:47Z
dc.descriptionWe briefly discuss the theory of epicyclic motion near rotating black holes and its relation to the origin of high frequency Quasi-Periodic Oscillations (QPOs) seen in many cases of accreting black hole binaries. We also point out some new frequency ratios predicted by the theory.
dc.descriptionTo appear in the Proceedings of the Eleventh Marcel Grossmann Meeting, Berlin, Germany, 23-29 Jule 2006, 3pp., World Scientific, Singapore (2007)
dc.identifierhttps://arxiv.org/abs/astro-ph/0612730
dc.identifierhttp://arxiv.org/abs/astro-ph/0612730
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/120895
dc.subjectAstrophysics
dc.titleEpicyclic Frequencies and Resonant Phenomena Near Black Holes: The Current Status
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