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

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

2008-11-28

arxiv.org/abs/0811.4705v1

RAA 9: 157-167, 2009

Astronomy and Astrophysics

Astrophysics

12 pages including 3 figures; to appear in Research in Astronomy and Astrophysics

Scientific paper

10.1088/1674-4527/9/2/005

We provide a 2.5-dimensional solution to a complete set of viscous hydrodynamical equations describing accretion-induced outflow and then plausible jet 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 inflow-outflow system essentially upholds the conservation laws. We provide a set of analytical family of solutions through the self-similar approach. The flow parameters of the disk-outflow system depend strongly on viscosity parameter \alpha and cooling factor f.

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