Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 370, Issue 2, Pages 975-980Publisher
OXFORD UNIV PRESS
DOI: 10.1111/j.1365-2966.2006.10524.x
Keywords
MHD; stars : formation; ISM : clouds
Categories
Ask authors/readers for more resources
Using 2D simulations, we study the formation of structures with a high-density contrast by magnetohydrodynamic waves in regions in which the ratio of thermal to magnetic pressure is small. The initial state is a uniform background perturbed by fast-mode wave. Our most significant result is that dense structures persist for far longer in a 2D simulation than in the 1D case. Once formed, these structures persist as long as the fast-mode amplitude remains high.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available