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Observation of triggering in the Milky Way

Published online by Cambridge University Press:  01 August 2006

L. Deharveng ,
A. Zavagno ,
B. Lefloch ,
J. Caplan  and
M. Pomarès
L. Deharveng
Affiliation:
Laboratoire d'Astrophysique de Marseille, 2 Place le Verrier, 13248 Marseille Cedex 4, France email: [email protected]
A. Zavagno
Affiliation:
Laboratoire d'Astrophysique de Marseille, 2 Place le Verrier, 13248 Marseille Cedex 4, France email: [email protected]
B. Lefloch
Affiliation:
Laboratoire d'Astrophysique de l'Observatoire de Grenoble
J. Caplan
Affiliation:
Laboratoire d'Astrophysique de Marseille, 2 Place le Verrier, 13248 Marseille Cedex 4, France email: [email protected]
M. Pomarès
Affiliation:
Laboratoire d'Astrophysique de Marseille, 2 Place le Verrier, 13248 Marseille Cedex 4, France email: [email protected]
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Abstract

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We show how the expansion of classical Galactic Hii regions can trigger massive-star formation via the collect & collapse process. We give examples of this process at work. We suggest that it also works in a turbulent medium.

Keywords

stars: formationstars: early-typeISM: Hii regions
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S237: Triggered Star Formation in a Turbulent ISM , August 2006 , pp. 212 - 216
Copyright
Copyright © International Astronomical Union 2007

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