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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2443
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dc.contributor.authorDas, S-
dc.contributor.authorChakrabarti, S. K-
dc.date.accessioned2008-06-18T11:11:24Z-
dc.date.available2008-06-18T11:11:24Z-
dc.date.issued2002-
dc.identifier.citationBASI, Vol. 30, No. 1, pp. 321 - 325en
dc.identifier.urihttp://hdl.handle.net/2248/2443-
dc.description.abstractShocks from around black holes as the matter slows down by centifugal barrier. At the shocks, kinetic energy is converted into thermal energy and hard-X rays, outflows etc. are produced which are observed. We compute the locations of these shocks analytically by using a set of approximations and found that they match very well with those obtained by numerical techniques. From the shock properties we compute QPO oscillation frequencies and outflow rate in the jets.en
dc.format.extent356135 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2002BASI...30..321Den
dc.subjectAccretionen
dc.subjectAccretion Disksen
dc.subjectBlack Hole Physicsen
dc.subjectHydrodynamicsen
dc.subjectShock Wavesen
dc.titleAnalytical study of standing shocks around black holeen
dc.typeArticleen
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