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hal.structure.identifierFORMATION STELLAIRE 2012
dc.contributor.authorBRAINE, J.
hal.structure.identifierInstitut de RadioAstronomie Millimétrique [IRAM]
dc.contributor.authorGRATIER, P.
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorCONTRERAS, Y.
hal.structure.identifierInstitut de Planétologie et d'Astrophysique de Grenoble [IPAG ]
dc.contributor.authorSCHUSTER, K. F.
hal.structure.identifierFORMATION STELLAIRE 2012
dc.contributor.authorBROUILLET, N.
dc.date.issued2012-10
dc.descriptionVizieR On-line Data Catalog: J/A+A/548/A52. Originally published in: 2012A&A...548A..52B
dc.description.abstractEnThe amount of H2 present in spiral galaxies remains unce particularly in the dim outer regions and in low-metallicity environments. We present high-resolution CO(1-0) observations with the Plateau de Bure interferometer of the most distant molecular cloud in the local group galaxy M33. The cloud is a single entity rather than a set of smaller clouds within the broad beam of the original single-dish observations. The interferometer and single-dish fluxes are very similar and the line widths are indistinguishable, despite the difference in beamsize. (2 data files).
dc.language.isoen
dc.subject.enGalaxies: nearby
dc.subject.enMolecular clouds
dc.title.enMolecular cloud formation in M 33 (Braine+, 2012)
dc.typeAutre document
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.page89052
hal.identifierhal-00787032
hal.version1
hal.popularnon
hal.audienceNon spécifiée
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00787032v1
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