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Triggering and the gravitational instability in shells and supershells

Published online by Cambridge University Press:  01 August 2006

Jan Palouš
Jan Palouš*
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic, Boční II 1401, 140 41 Prague 4, Czech Republic email: palous@ig.cas.cz
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Abstract

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The gravitational instability of shells and supershells and its relevance to the triggering of the star formation in a turbulent ISM is discussed. The IMF of the self-gravitating clumps formed out of shells is computed and triggering time is compared with the shell dissolution time due to chaotic motions.

Keywords

shock wavesturbulenceISM: bubblesISM: cloudsstars: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S237: Triggered Star Formation in a Turbulent ISM , August 2006 , pp. 114 - 118
Copyright
Copyright © International Astronomical Union 2007

References

Brinks, E. 2006, this volumeGoogle Scholar
Ehlerová, S. 2006, this volumeGoogle Scholar
Ehlerová, J., & Palouš, J. 2005, A&A 437, 101Google Scholar
Elmegreen, B.G., & Elmegreen, D. 1978 ApJ 220, 1051CrossRefGoogle Scholar
Elmegreen, B.G., & Lada, Ch. 1978, ApJ 214, 725CrossRefGoogle Scholar
Elmegreen, B.G., & Scalo, J. 2004, ARA&A 42, 211Google Scholar
Larson, R.B. 1981, MNRAS 194, 809CrossRefGoogle Scholar
Palouš, J., Ehlerová, S., & Wünsch, R. 2003 Astrophys. and Space Sci. 284, 873CrossRefGoogle Scholar
Scalo, J., & Elmegreen, B.G. 2004, ARA&A 42, 275Google Scholar
Stanimirovic, S. 2006, this volumeGoogle Scholar