High mass star and cluster formation: new insights from Herschel
hal.structure.identifier | Procédés, Matériaux et Energie Solaire [PROMES] | |
dc.contributor.author | FRÉDÉRIQUE, Motte | |
hal.structure.identifier | FORMATION STELLAIRE 2015 | |
dc.contributor.author | BONTEMPS, Sylvain | |
dc.contributor.author | HILL, Tracey, | |
dc.date.issued | 2015-08 | |
dc.date.conference | 2015-01-04 | |
dc.description.abstractEn | 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. | |
dc.language.iso | en | |
dc.title.en | High mass star and cluster formation: new insights from Herschel | |
dc.type | Communication dans un congrès | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO] | |
bordeaux.page | 58385 | |
bordeaux.volume | 22 | |
bordeaux.conference.title | 2015IAUGA..2258385M - IAU General Assembly, Meeting #29, #2258385 - held 4-8 January 2015 in Seattle, USA | |
bordeaux.country | US | |
bordeaux.conference.city | Seattle | |
bordeaux.peerReviewed | oui | |
hal.identifier | hal-01197413 | |
hal.version | 1 | |
hal.invited | non | |
hal.proceedings | non | |
hal.conference.end | 2015-01-08 | |
hal.popular | non | |
hal.audience | Internationale | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-01197413v1 | |
bordeaux.COinS | ctx_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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