Wind induced instabilities in accretion flow around black holes

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