Vertically Self-Gravitating ADAFs in the Presence of Toroidal Magnetic Field
arXiv:1110.2941 · doi:10.1007/s10509-011-0894-4
Abstract
Force due to the self-gravity of the disc in the vertical direction is considered to study its possible effects on the structure of a magnetized advection-dominated accretion disc. We present steady-sate self similar solutions for the dynamical structure of such a type of the accretion flows. Our solutions imply reduced thickness of the disc because of the self-gravity. It also imply that the thickness of the disc will increase by adding the magnetic field strength.
arXiv commentAccepted for publication in Astrophysics and Space Sciences
References in corpus (14)
- Advection-Dominated Accretion: A Self-Similar Solution
- On the Fate of Gas Accreting at a Low Rate onto a Black Hole
- Advection-Dominated Accretion and the Spectral States of Black Hole X-Ray Binaries: Application to Nova Muscae 1991
- Nuclear Activity in Nearby Galaxies
- Advection-Dominated Accretion: Self-Similarity and Bipolar Outflows
- Hydrodynamical Non-radiative Accretion Flows in Two-Dimensions
- Global Structure of Three Distinct Accretion Flows and Outflows around Black Holes through Two-Dimensional Radiation-Magnetohydrodynamic Simulations
- Slim Disk Model for Ultra-Luminous X-Ray Sources
- Self-Similar Solutions for ADAF with Toroidal Magnetic Fields
- The Influences of Outflow on the Dynamics of Inflow
- Self-Similar Solution of Hot Accretion Flows with Ordered Magnetic Field and Outflow
- The Effects of Thermal Conduction on the ADAF with a Toroidal Magnetic Field
- Hydrodynamical wind on a magnetized ADAF with thermal conduction
- Time-dependent evolution of quasi-spherical, self-gravitating accretion flow