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The generation of dense cores and substructure within them by MHD waves

Published online by Cambridge University Press:  01 August 2006

S. Van Loo ,
S. A. E. G. Falle  and
T. W. Hartquist
S. Van Loo
Affiliation:
University of Leeds, Leeds LS9 JT, UK email: svenvl@ast.leeds.ac.uk
S. A. E. G. Falle
Affiliation:
University of Leeds, Leeds LS9 JT, UK email: svenvl@ast.leeds.ac.uk
T. W. Hartquist
Affiliation:
University of Leeds, Leeds LS9 JT, UK email: svenvl@ast.leeds.ac.uk
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Abstract

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By using 2D simulations, we examine the generation of dense cores and substructures by magnetosonic waves. We find that the excitation of slow-mode waves by fast-mode waves produces these high-density structures.

Keywords

MHDstars: formationISM: clouds
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S237: Triggered Star Formation in a Turbulent ISM , August 2006 , pp. 486
Copyright
Copyright © International Astronomical Union 2007

References

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