Lim, A.J., Falle, S.A.E.G. and Hartquist, T.W. (2005) The production of magnetically dominated star-forming regions. The Astrophysical Journal, 632 (2). L91-L94. ISSN 0004-637X
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.
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.
|Copyright, Publisher and Additional Information:||© 2005 The American Astronomical Society|
|Institution:||The University of Leeds|
|Academic Units:||The University of Leeds > Faculty of Maths and Physical Sciences (Leeds) > School of Physics and Astronomy (Leeds)
The University of Leeds > Faculty of Maths and Physical Sciences (Leeds) > School of Mathematics (Leeds) > Applied Mathematics (Leeds)
|Depositing User:||Repository Assistant|
|Date Deposited:||08 Jun 2006|
|Last Modified:||06 Jun 2014 18:44|
|Publisher:||The University of Chicago Press|