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hal.structure.identifierProcédés, Matériaux et Energie Solaire [PROMES]
dc.contributor.authorFRÉDÉRIQUE, Motte
hal.structure.identifierFORMATION STELLAIRE 2015
dc.contributor.authorBONTEMPS, Sylvain
dc.contributor.authorHILL, Tracey,
dc.date.issued2015-08
dc.date.conference2015-01-04
dc.description.abstractEnThe 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.
dc.language.isoen
dc.title.enHigh mass star and cluster formation: new insights from Herschel
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
bordeaux.page58385
bordeaux.volume22
bordeaux.conference.title2015IAUGA..2258385M - IAU General Assembly, Meeting #29, #2258385 - held 4-8 January 2015 in Seattle, USA
bordeaux.countryUS
bordeaux.conference.citySeattle
bordeaux.peerReviewedoui
hal.identifierhal-01197413
hal.version1
hal.invitednon
hal.proceedingsnon
hal.conference.end2015-01-08
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01197413v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2015-08&rft.volume=22&rft.spage=58385&rft.epage=58385&rft.au=FR%C3%89D%C3%89RIQUE,%20Motte&BONTEMPS,%20Sylvain&HILL,%20Tracey,&rft.genre=unknown


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