Back to Volume
Paper: Magnetic Fields and the Formation of Cores and Disks
Volume: 476, New Trends in Radio Astronomy in the ALMA Era
Page: 103
Authors: Basu, S.; Bailey, N. D.; Dapp, W. B.
Abstract: We review recent results of non-ideal magnetohydrodynamic models for the fragmentation of molecular clouds and the collapse of cloud cores to form protostar-disk systems. Thin-disk models can elucidate many aspects of the physical problem and allow the calculation of large dynamic range of time and length scales.
Back to Volume