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Results of the IRAM M33 Large Program

hal.structure.identifierFORMATION STELLAIRE 2013
dc.contributor.authorBRAINE, J.
dc.contributor.authorSCHUSTER, Karl
dc.contributor.authorGRATIER, P.
hal.structure.identifierAMOR 2013
dc.contributor.authorDRUARD, C.
dc.date.issued2013-03
dc.date.conference2012
dc.description.abstractEnA very sensitive survey of the CO(2-1) emission of the entire disk of the Local Group galaxy M 33 is virtually complete. Hundreds of clouds down to a mass of 10000M&sun; are detected and we show that the cloud mass function (assuming a constant ratio between CO emission and H2 mass) steepens away from the center of M 33. Through comparison with dust emission and cloud Virial masses, we estimate a N(H2)/I CO factor roughly twice Galactic.
dc.language.isoen
dc.subject.engalaxies: individual (M33)
dc.subject.enLocal Group
dc.subject.engalaxies: evolution
dc.subject.engalaxies: ISM
dc.subject.enISM: clouds
dc.subject.enstars: formation
dc.title.enResults of the IRAM M33 Large Program
dc.typeCommunication dans un congrès
dc.identifier.doi10.1017/S1743921313000793
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
bordeaux.page135-138
bordeaux.volume292
bordeaux.countryCN
bordeaux.conference.cityBeijing
bordeaux.peerReviewedoui
hal.identifierhal-00822738
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00822738v1
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