Issue |
EAS Publications Series
Volume 34, 2009
Astronomy in the Submillimeter and Far Infrared Domains with the Herschel Space Observatory
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Page(s) | 195 - 211 | |
DOI | https://doi.org/10.1051/eas:0934014 | |
Published online | 20 December 2008 |
Astronomy in the Submillimeter and Far Infrared Domains with the Herschel Space Observatory
L. Pagani and M. Gerin (eds)
EAS Publications Series, 34 (2009) 195-211
L. Pagani and M. Gerin (eds)
EAS Publications Series, 34 (2009) 195-211
Our knowledge of high-mass star formation at the dawn of Herschel
1
Laboratoire AIM, CEA/DSM, CNRS, Université Paris Diderot, DAPNIA/SAp, CEA-Saclay, 91191 Gif-sur-Yvette Cedex, France
2
École Normale Supérieure, 24 rue Lhomond, 75005 Paris, France
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.
© EAS, EDP Sciences, 2009