Skip to main content
Article thumbnail
Location of Repository

The production of magnetically dominated star-forming regions

By A.J. Lim, S.A.E.G. Falle and T.W. Hartquist

Abstract

We consider the dynamical evolution of an interstellar cloud that is initially in thermal equilibrium in the warm phase and is then subjected to a sudden increase in the pressure of its surroundings. We find that if the initial plasma β of the cloud is of order unity, then there is a considerable period during which the material in the cloud both has a small β and is in the thermally unstable temperature range.\ud \ud These conditions are not only consistent with observations of star-forming regions but also ideally suited to the production of density inhomogeneities by magnetohydrodynamic waves. The end result should be a cloud whose size and average density are typical of Giant Molecular Clouds (GMCs) and that contains denser regions whose densities are in the range inferred for the translucent clumps in GMCs

Publisher: The University of Chicago Press
Year: 2005
OAI identifier: oai:eprints.whiterose.ac.uk:1264

Suggested articles


To submit an update or takedown request for this paper, please submit an Update/Correction/Removal Request.