Vertically Self-Gravitating ADAFs in the Presence of Toroidal Magnetic Field

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.

Accepted for publication in Astrophysics and Space Sciences

References in corpus (3)

• Global Structure of Three Distinct Accretion Flows and Outflows around Black Holes through Two-Dimensional Radiation-Magnetohydrodynamic Simulations
• Self-Similar Solution of Hot Accretion Flows with Ordered Magnetic Field and Outflow
• Hydrodynamical wind on a magnetized ADAF with thermal conduction

Cited by in corpus (2)

• Hydrodynamical wind on vertically self-gravitating ADAFs in the presence of toroidal magnetic field
• The effects of toroidal magnetic field on the vertical structure of hot accretion flows