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HOBYS and W43, two more steps towards a Galaxy-wide understanding of star formation

hal.structure.identifierProcédés, Matériaux et Energie Solaire [PROMES]
dc.contributor.authorMOTTE, Frederique,
hal.structure.identifierFORMATION STELLAIRE 2015
dc.contributor.authorBONTEMPS, Sylvain
dc.contributor.authorNGUYEN LUONG, Quang,
dc.date.issued2015-08
dc.date.conference2015-01-04
dc.description.abstractEnThe HOBYS key program allows to statistically study the formation of 10-20 Msun stars in molecular complexes from the first Galactic arm toward us. HOBYS therefore starts to measure the star formation rate of the Milky Way on 1-100 pc scales. The much more extreme W43 molecular complex is located at the tip of the long bar of the Milky Way and forms stars up to 50 Msun. It displays an intense star formation activity, which may originate from its dynamical cloud formation. The HOBYS and W43 surveys are necessary steps towards Galaxy-wide studies of high-mass star formation.
dc.language.isoen
dc.title.enHOBYS and W43, two more steps towards a Galaxy-wide understanding of star formation
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
bordeaux.page58331
bordeaux.volume22
bordeaux.countryUS
bordeaux.conference.citySeattle
bordeaux.peerReviewedoui
hal.identifierhal-01197416
hal.version1
hal.invitednon
hal.proceedingsnon
hal.conference.end2015-01-08
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01197416v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2015-08&rft.volume=22&rft.spage=58331&rft.epage=58331&rft.au=MOTTE,%20Frederique,&BONTEMPS,%20Sylvain&NGUYEN%20LUONG,%20Quang,&rft.genre=unknown


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