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.
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Mosallanezhad, A., Abbassi, S., Shadmehri, M. et al. Vertically self-gravitating ADAFs in the presence of toroidal magnetic field. Astrophys Space Sci 337, 703–710 (2012). https://doi.org/10.1007/s10509-011-0894-4
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DOI: https://doi.org/10.1007/s10509-011-0894-4