2.5-dimensional solution of the advective accretion disk: a self-similar approach

dc.contributor.author	Ghosh, S
dc.contributor.author	Mukhopadhyay, B
dc.date.accessioned	2009-05-21T16:39:16Z
dc.date.available	2009-05-21T16:39:16Z
dc.date.issued	2009-02
dc.identifier.citation	Research in Astronomy and Astrophysics, Vol. 9, No. 2, pp. 157 - 167	en
dc.identifier.issn	1674-4527
dc.identifier.uri	http://hdl.handle.net/2248/4485
dc.description.abstract	We provide a 2.5-dimensional solution to a complete set of viscous hydrodynamical equations describing accretion-induced outflows and plausible jets around black holes/compact objects. We prescribe a self-consistent advective disk-outflow coupling model, which explicitly includes the information of vertical flux. Inter-connecting dynamics of an inflow-outflow system essentially upholds the conservation laws. We provide a set of analytical family of solutions through a self-similar approach. The flow parameters of the disk-outflow system depend strongly on the viscosity parameter α and the cooling factor f.	en
dc.language.iso	en	en
dc.publisher	Institute of Physics	en
dc.relation.uri	http://arxiv.org/abs/0811.4705	en
dc.relation.uri	http://dx.doi.org/10.1088/1674-4527/9/2/005	en
dc.rights	© Institute of Physics	en
dc.subject	Accretion
dc.subject	Accretion disk
dc.subject	Black hole physics
dc.subject	Hydrodynamics
dc.subject	Galaxies: jets
dc.title	2.5-dimensional solution of the advective accretion disk: a self-similar approach	en
dc.type	Article	en