Role of thermal conduction in an advective accretion with bipolar outflows
arXiv:1309.5710 · doi:10.1093/mnras/stt1762
Abstract
Steady-state advective accretion flows in the presence of thermal conduction are studied. All three components of velocity in a spherical coordinates are considered and the flow displays both inflowing and outflowing regions according to our similarity solutions. Thermal conductivity provides latitudinal energy transport and so, the flow rotates more slowly and becomes hotter with increasing thermal conductivity coefficient. We also show that opening angle of the outflow region decreases as thermal conduction becomes stronger.
6 pages, 4 figures, accepted for publication in MNRAS
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Cited by in corpus (6)
- The Effect of Large Scale Magnetic Field on Outflow in ADAFs: an Odd Symmetry Configuration
- Global Transonic Solution of Hot Accretion Flow with Thermal Conduction
- Two-dimensional Inflow-Wind Solution of Hot Accretion Flow. I. Hydrodynamics
- Self-similar Solution of Hot Accretion Flow with Thermal Conduction and Anisotropic Pressure
- Self-similar solution of hot accretion flow: the role of kinematic viscosity coefficient
- Fourier analysis of advection-dominated accretion flows