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TWO-DIMENSIONAL ADAPTIVE CODE FOR SIMULATION OF ASTROPHYSICAL MAGNETOHYDRODYNAMIC FLOWS

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Integrated adaptive mesh for simulations of two-dimensional (2D) self-gravitating, axially symmetric magnetohydrodynamic (MHD) flows in spherical coordinates is constructed and a new adaptive numerical 2D MHD code is developed. This code allows us to simulate efficiently the gravitational collapse of magnetized rotating protostellar clouds. Illustrative test computations are presented.
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Keywords: Collapse; Interstellar medium; Magnetohydrodynamics; Numerical methods; Star formation

Document Type: Research Article

Affiliations: 1: Chelyabinsk State University, Br. Kashirinykh 129, Chelyabinsk 454021, Russia 2: Keldysh Institute of Applied Mathematics, Miusskaya Square 4, Moscow 125047, Russia

Publication date: 2003-06-01

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