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hal.structure.identifierLaboratoire de Radioastronomie [LRA]
dc.contributor.authorBELLOCHE, Arnaud
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorPARISE, Berengere
hal.structure.identifierLaboratoire de Physique des Lasers [LPL]
dc.contributor.authorSCHULLER, Frederic
dc.contributor.authorANDRE, Philippe
hal.structure.identifierFORMATION STELLAIRE 2013
dc.contributor.authorBONTEMPS, Sylvain
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorMENTEN, Karl
dc.date.conference2013
dc.description.abstractEnThe nearby Chamaeleon molecular cloud complex is an excellent laboratory for studying the process of low-mass star formation because it consists of three clouds with very different properties. Chamaeleon III does not show any sign of star formation, while star formation has been very active in Chamaeleon I and may already be finishing. We will present the results of an unbiased continuum survey for starless and protostellar cores performed toward both clouds with the Large APEX Bolometer Array (LABOCA) at 870 microns. We will discuss the dynamical state and fate of the starless cores detected in both clouds.
dc.language.isoen
dc.title.enThe Fate of Star Formation in Chamaeleon I and III
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
bordeaux.countryDE
bordeaux.conference.cityHeidelberg
bordeaux.peerReviewedoui
hal.identifierhal-00880547
hal.version1
hal.invitednon
hal.proceedingsnon
hal.popularnon
hal.audienceNon spécifiée
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00880547v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.au=BELLOCHE,%20Arnaud&PARISE,%20Berengere&SCHULLER,%20Frederic&ANDRE,%20Philippe&BONTEMPS,%20Sylvain&rft.genre=unknown


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