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NUMERICAL SIMULATION OF PROTOSTAR FORMATION IN MAGNETIZED MOLECULAR CLOUD CORES

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The two-dimensional numerical simulations of magnetized molecular cloud collapse has been done using integrated adaptive mesh in spherical coordinates. To take into account non-isothermality of late stages of collapse, we use a kind of "parametrical" approach to the radiative transfer through the cloud. Several numerical models are presented.
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Keywords: Collapse; Interstellar medium; MHD; Molecular cloud cores; Numerical simulation; Star formation

Document Type: Research Article

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

Publication date: 2003-02-01

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