Numerical Simulation of Protostar Formation in Magnetized Molecular Cloud Cores

Details Numerical Simulation of Protostar Formation in Magnetized Molecular Cloud Cores Numerical Simulation of Protostar Formation in Magnetized Molecular Cloud Cores

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003a%26at...22...11d&link_type=abstract

Astronomical and Astrophysical Transactions, vol. 22, Issue 1, p.11-14

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Scientific paper

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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