@osso73

Star formation in molecular cloud cores

, , and . Star Forming Regions, volume 115 of IAU Symposium, page 417-433. (January 1987)

Abstract

A scenario for star formation is described based on the assumption that magnetic fields play an important dynamical role in the interstellar medium. Particular attention is given to the evolution of a molecular cloud which is initially subcritical but which has a mass (supported by a combination of magnetic fields and sub-Alfvenic 'turbulence') that much exceeds the Jeans mass computed on the basis of the average density and temperature. It is argued that the magnetic support of such an object will automatically lead to the production of many small cores.

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