High mass star and cluster formation: new insights from Herschel

Frederique, Motte 1 S. Bontemps 2 Tracey, Hill
2 FORMATION STELLAIRE 2015
LAB - Laboratoire d'Astrophysique de Bordeaux [Pessac], UB - Université de Bordeaux, INSU - CNRS - Institut national des sciences de l'Univers , CNRS - Centre National de la Recherche Scientifique
Abstract : The HOBYS key program essentially imaged with Herschel all of the regions forming OB-type stars at distances less than 3 kpc from the Sun. This survey allows to statistically study the formation of 10-20 Msun stars and confirms that high-mass pre-stellar cores do not exist. HOBYS also reveals mini-starburst cloud ridges, which have high mean densities and are the privileged sites for the formation of high-mass stars.
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Communication dans un congrès
2015IAUGA.2258385M - IAU General Assembly, Meeting #29, #2258385 - held 4-8 January 2015 in Seattle, USA, Jan 2015, Seattle, United States. 22, pp.58385, 2015
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https://hal.archives-ouvertes.fr/hal-01197413
Contributeur : Marie-Paule Pomies <>
Soumis le : vendredi 11 septembre 2015 - 16:13:40
Dernière modification le : jeudi 8 septembre 2016 - 15:20:43

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Frederique, Motte, S. Bontemps, Tracey, Hill. High mass star and cluster formation: new insights from Herschel. 2015IAUGA.2258385M - IAU General Assembly, Meeting #29, #2258385 - held 4-8 January 2015 in Seattle, USA, Jan 2015, Seattle, United States. 22, pp.58385, 2015. <hal-01197413>

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