NUMERICAL SIMULATION OF PROTOSTAR FORMATION IN MAGNETIZED MOLECULAR CLOUD CORES
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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Document Type: Research Article
Publication date: 2003-02-01