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• W3100101968 abstract "We solve the set of hydrodynamic (HD) equations for optically thin Advection Dominated Accretion Flows (ADAFs) by assuming radially self-similar in spherical coordinate system $ (r, theta, phi) $. The disk is considered to be steady state and axi-symmetric. We define the boundary conditions at the pole and the equator of the disk and to avoid singularity at the rotation axis, the disk is taken to be symmetric with respect to this axis. Moreover, only the $ tau_{r phi} $ component of viscous stress tensor is assumed and we have set $ v_{theta} = 0 $. The main purpose of this study is to investigate the variation of dynamical quantities of the flow in the vertical direction by finding an analytical solution. As a consequence, we found that the advection parameter, $ f^{adv} $, varies along the $ theta $ direction and reaches to its maximum near the rotation axis. Our results also show that, in terms of no-outflow solution, thermal equilibrium still exists and consequently advection cooling can balance viscous heating." @default.
• W3100101968 created "2020-11-23" @default.
• W3100101968 creator A5010660545 @default.
• W3100101968 creator A5053999183 @default.
• W3100101968 date "2015-08-10" @default.
• W3100101968 modified "2023-10-16" @default.
• W3100101968 title "VERTICAL STRUCTURE OF ADVECTION-DOMINATED ACCRETION FLOWS" @default.
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• W3100101968 doi "https://doi.org/10.1088/0004-637x/809/1/54" @default.
• W3100101968 hasPublicationYear "2015" @default.
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