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Our knowledge of high-mass star formation at the dawn of Herschel

Published online by Cambridge University Press:  20 December 2008

L. Pagani ,
M. Gerin ,
F. Motte  and
P. Hennebelle
F. Motte
Affiliation:
Laboratoire AIM, CEA/DSM, CNRS, Université Paris Diderot, DAPNIA/SAp, CEA-Saclay, 91191 Gif-sur-Yvette Cedex, France
P. Hennebelle
Affiliation:
École Normale Supérieure, 24 rue Lhomond, 75005 Paris, France
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Abstract

We review the theories and observations of high-mass star formation emphasizing the differences with those of low-mass star formation. We hereafter describe the progress expected to be achieved with Herschel, thanks notably to Key Programmes dedicated to the earliest phases of high-mass star formation.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 34: Astronomy in the Submillimeter and Far Infrared Domains with the Herschel Space Observatory , 2009 , pp. 195 - 211
Copyright
© EAS, EDP Sciences, 2009

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