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Observations of star formation triggered by H ii regions

Published online by Cambridge University Press:  27 April 2011

Lise Deharveng  and
Annie Zavagno
Lise Deharveng
Affiliation:
Laboratoire d'Astrophysique de Marseille (UMR 6110, CNRS & Université de Provence), 38 rue F. Joliot-Curie, 13388 Marseille Cedex 13, France email: lise.deharveng@oamp.fr
Annie Zavagno
Affiliation:
Laboratoire d'Astrophysique de Marseille (UMR 6110, CNRS & Université de Provence), 38 rue F. Joliot-Curie, 13388 Marseille Cedex 13, France email: lise.deharveng@oamp.fr
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Abstract

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Observations show that expanding H ii regions may trigger star formation. We discuss several aspects of this type of star formation, and try to estimate its prevalence. We show how LMC H ii regions may help us to understand what we see in our Galaxy.

Keywords

stars: formationISM: H ii regionsISM: bubblesinfrared: ISMinfrared: stars
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S270: Computational Star Formation , May 2010 , pp. 239 - 246
Copyright
Copyright © International Astronomical Union 2011

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