High mass star and cluster formation: new insights from Herschel
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en
Communication dans un congrès
Ce document a été publié dans
2015IAUGA..2258385M - IAU General Assembly, Meeting #29, #2258385 - held 4-8 January 2015 in Seattle, USA, 2015-01-04, Seattle. 2015-08, vol. 22, p. 58385
Résumé en anglais
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 ...Lire la suite >
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.< Réduire
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