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Collapse and Fragmentation of Rotating Magnetized Clouds. I. Magnetic Flux - Spin Relation
Monthly Notices of the Royal Astronomical Society, no. 2 (2005): 369-381
EI WOS
摘要
We discuss the evolution of the magnetic flux density and angular velocity in a molecular cloud core, on the basis of three-dimensional numerical simulations, in which a rotating magnetized cloud fragments and collapses to form a very dense optically thick core of >5 × 1010 cm−3. As the density increases towards the formation of the optic...更多
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