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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2437
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dc.contributor.authorAcharya, K-
dc.contributor.authorChakrabarti, S. K-
dc.contributor.authorMolteni, D-
dc.date.accessioned2008-06-16T12:21:23Z-
dc.date.available2008-06-16T12:21:23Z-
dc.date.issued2002-
dc.identifier.citationBASI, Vol. 30, No. 1, pp. 317 - 320en
dc.identifier.urihttp://hdl.handle.net/2248/2437-
dc.description.abstractWe identify a new type of instability of the accrelation flow which is formed due to interaction of the outgoing winds with the incoming flow. Mainly due to shear instability, the flow oscillates around the equatorial plane. We show that in the shocks are formed in accretion flows, this new type of oscillation persists along with the usual radial oscillation.en
dc.format.extent357597 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2002BASI...30..317Aen
dc.subjectAccretionen
dc.subjectAccretion Disksen
dc.subjectBlack Hole Physicsen
dc.subjectHydrodynamicsen
dc.subjectShock Wavesen
dc.titleWind induced instabilities in accretion flow around black holesen
dc.typeArticleen
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