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Magnetic Fields and the Formation of Cores and Disks

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.

preprint2013arXivOpen access
Shantanu BasuNicole D. BaileyWolf B. Dapp
astro-ph.GAastro-ph.SR
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Open access3 authors2 topics
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Shantanu BasuNicole D. BaileyWolf B. Dapp

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