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Wind induced instabilities in accretion flow around black holes

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dc.contributor.author Acharya, K
dc.contributor.author Chakrabarti, S. K
dc.contributor.author Molteni, D
dc.date.accessioned 2008-06-16T12:21:23Z
dc.date.available 2008-06-16T12:21:23Z
dc.date.issued 2002
dc.identifier.citation BASI, Vol. 30, No. 1, pp. 317 - 320 en
dc.identifier.uri http://hdl.handle.net/2248/2437
dc.description.abstract We 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.extent 357597 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Astronomical Society of India en
dc.relation.uri http://adsabs.harvard.edu/abs/2002BASI...30..317A en
dc.subject Accretion en
dc.subject Accretion Disks en
dc.subject Black Hole Physics en
dc.subject Hydrodynamics en
dc.subject Shock Waves en
dc.title Wind induced instabilities in accretion flow around black holes en
dc.type Article en

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