Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-26T18:47:22.984Z Has data issue: false hasContentIssue false
  • English
  • Français

The fragmentation of expanding shells – limitations of the thin-shell model

Published online by Cambridge University Press:  18 January 2010

Jim Dale ,
Richard Wünsch ,
Jan Palouš  and
Ant Whitworth
Jim Dale
Affiliation:
Astronomical Institute, AVCR, Prague, Czech Republic
Richard Wünsch
Affiliation:
Astronomical Institute, AVCR, Prague, Czech Republic
Jan Palouš
Affiliation:
Astronomical Institute, AVCR, Prague, Czech Republic
Ant Whitworth
Affiliation:
School of Physics and Astronomy, Cardiff University, Cardiff, UK
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We study the fragmentation of expanding shells in the context of the linear thin-shell analysis. We simulate shell fragmentation using the flash AMR code and a variant of the Benz SPH code.

Keywords

stars: formationISM: bubbles
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S266: Star clusters: basic galactic building blocks throughout time and space , August 2009 , pp. 375
Copyright
Copyright © International Astronomical Union 2010