High mass star and cluster formation: new insights from Herschel - Archive ouverte HAL Accéder directement au contenu
Communication Dans Un Congrès Année : 2015

High mass star and cluster formation: new insights from Herschel

Sylvain Bontemps
Tracey, Hill
  • Fonction : Auteur

Résumé

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.
Fichier non déposé

Dates et versions

hal-01197413 , version 1 (11-09-2015)

Identifiants

Citer

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⟩
57 Consultations
0 Téléchargements

Partager

Gmail Facebook X LinkedIn More