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A class of self-gravitating, magnetized accretion disks

Mohsen Shadmehri·Fazeleh Khajenabi
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Abstract

The steady-state structure of self-gravitating, magnetized accretion disks is studied using a set of self-similar solutions which are appropriate in the outer regions. The disk is assumed to be isothermal and the magnetic field outside of the disk is treated in a phenomenological way. However, the internal field is determined self-consistently. The behaviour of the solutions are investigated by changing the input parameters of the model, i.e. mass accretion rate, coefficients of viscosity and resistivity, and the magnetic field configuration.

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Mohsen Shadmehri, Fazeleh Khajenabi. 2005-09-28. A class of self-gravitating, magnetized accretion disks. https://doi.org/10.1086/498390

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