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Conference papers

High mass star and cluster formation: new insights from Herschel

Frederique, Motte 1 Sylvain Bontemps 2 Tracey, Hill 
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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Submitted on : Friday, September 11, 2015 - 4:13:40 PM
Last modification on : Tuesday, December 21, 2021 - 3:26:04 PM




Frederique, Motte, Sylvain 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. pp.58385. ⟨hal-01197413⟩



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