Dynamics of Magnetized Spherical Accretion Flows
Roman V. Shcherbakov
TL;DR
This paper investigates the behavior of magnetized spherical accretion flows, focusing on their transonic properties and the role of magnetic fields in shaping the flow dynamics.
Contribution
It introduces a self-consistent model of transonic accretion flows that incorporates random magnetic fields, advancing understanding of magnetized accretion processes.
Findings
Magnetic fields significantly influence flow transonicity.
Self-consistent magnetic field treatment alters accretion flow structure.
Results provide insights into astrophysical accretion phenomena.
Abstract
Transonic accretion flow with self-consistent treatment of random magnetic field is presented.
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