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From ATLASGAL to SEDIGISM: Towards a Complete 3D View of the Dense Galactic Interstellar Medium

hal.structure.identifierLaboratoire de Physique des Lasers [LPL]
dc.contributor.authorSCHULLER, F.,
hal.structure.identifierMars Desert Research Station [MDRS]
dc.contributor.authorURQUHART, J.,
hal.structure.identifierDepartamento de Astronomia [DAS]
dc.contributor.authorBRONFMAN, L.,
dc.contributor.authorCSENGERI, T.,
hal.structure.identifierFORMATION STELLAIRE 2016
dc.contributor.authorBONTEMPS, Sylvain
dc.contributor.authorDUARTE-CABRAL, A.,
dc.contributor.authorGIANNETTI, A.,
hal.structure.identifierEuropean Southern Observatory [ESO]
dc.contributor.authorGINSBURG, A.,
dc.contributor.authorHENNING, T.,
dc.contributor.authorIMMER, K.,
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorLEURINI, S.,
dc.contributor.authorMATTERN, M.,
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorMENTEN, K.,
hal.structure.identifierCNR Istituto per la Protezione Sostenibile delle Piante [Torino, Italia] [IPSP]
dc.contributor.authorMOLINARI, S.,
dc.contributor.authorMULLER, E.,
hal.structure.identifierINAF - Osservatorio Astrofisico di Arcetri [OAA]
dc.contributor.authorSÁNCHEZ-MONGE, A.,
dc.contributor.authorSCHISANO, E.,
hal.structure.identifierUniversity of Oxford
dc.contributor.authorSURI, S.,
hal.structure.identifierEuropean Southern Observatory [ESO]
dc.contributor.authorTESTI, L.,
hal.structure.identifierKey Laboratory of Photobiology
dc.contributor.authorWANG, K.,
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorWYROWSKI, F.,
hal.structure.identifierLaboratoire d'Astrophysique de Marseille [LAM]
dc.contributor.authorZAVAGNO, Annie
dc.date.issued2016-09
dc.identifier.issn0722-6691
dc.description.abstractEnThe ATLASGAL survey has provided the first unbiased view of the inner Galactic Plane at sub-millimetre wavelengths. This is the largest ground-based survey of its kind to date, covering 420 square degrees at a wavelength of 870 µm. The reduced data, consisting of images and a catalogue of > 104 compact sources, are available from the ESO Science Archive Facility through the Phase 3 infrastructure. The extremely rich statistics of this survey initiated several follow-up projects, including spectroscopic observations to explore molecular complexity and high angular resolution imaging with the Atacama Large Millimeter/submillimeter Array (ALMA), aimed at resolving individual protostars. The most extensive follow-up project is SEDIGISM, a 3D mapping of the dense interstellar medium over a large fraction of the inner Galaxy. Some notable results of these surveys are highlighted.
dc.language.isoen
dc.publisherEuropean Southern Observatory
dc.title.enFrom ATLASGAL to SEDIGISM: Towards a Complete 3D View of the Dense Galactic Interstellar Medium
dc.typeArticle de revue
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA]
bordeaux.journalThe Messenger
bordeaux.page27 - 33
bordeaux.volume165
bordeaux.peerReviewednon
hal.identifierhal-01372251
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01372251v1
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