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The Next Generation of High-Mass Stars and Clusters Traced by ATLASGAL

hal.structure.identifierLaboratoire de Physique des Lasers [LPL]
dc.contributor.authorSCHULLER, Frédéric
dc.contributor.authorMENTEN, Karl M.
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorWYROWSKI, Friedrich
dc.contributor.authorCONTRERAS, Yanett
dc.contributor.authorCSENGERI, Timea
dc.contributor.authorURQUHART, James S.
dc.contributor.authorWIENEN, Marion
dc.contributor.authorBEUTHER, Henrik
hal.structure.identifierFORMATION STELLAIRE 2014
dc.contributor.authorBONTEMPS, Sylvain
dc.contributor.authorBRONFMAN, Leonardo
hal.structure.identifierObservatoire Astronomique de Marseille Provence [OAMP]
dc.contributor.authorDEHARVENG, Lise
hal.structure.identifierMax-Planck-Institut für Astronomie [MPIA]
dc.contributor.authorHENNING, Thomas
hal.structure.identifierINAF - Osservatorio Astrofisico di Arcetri [OAA]
dc.contributor.authorWALMSLEY, Malcolm
hal.structure.identifierLaboratoire d'Astrophysique de Marseille [LAM]
dc.contributor.authorZAVAGNO, Annie
dc.date.issued2014
dc.date.conference2012
dc.identifier.issn1570-6591
dc.description.abstractEnThe Atacama Pathfinder Experiment (APEX) telescope is ideally located to observe the inner part of our Galaxy. With its good sensitivity, the LABOCA bolometer array can map hundreds of square degrees at λ = 870 μ m λ = 870 \upmu m in a reasonable time. ATLASGAL, the APEX Telescope Large Area Survey of the Galaxy, covers 420 deg2 of the inner Galactic plane, with a typical rms noise of 50 mJy/beam. The data reveal thousands of compact sources, as well as giant molecular complexes and large scale filamentary structures. Many follow-up projects are ongoing, and more are planned e.g. with ALMA.
dc.language.isoen
dc.publisherSpringer
dc.source.title2014ASSP...36..421S - The Labyrinth of Star Formation, held in Greece, june 2012, Astrophysics and Space Science Proceedings, Volume 36. ISBN 978-3-319-03040-1. Springer International Publishing Switzerland, p. 421, 2014
dc.subject.enPhysics
dc.title.enThe Next Generation of High-Mass Stars and Clusters Traced by ATLASGAL
dc.typeCommunication dans un congrès
dc.identifier.doi10.1007/978-3-319-03041-8_84
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.journalAstrophysics and Space Science Proceedings
bordeaux.page421
bordeaux.volume36
bordeaux.countryGR
bordeaux.title.proceeding2014ASSP...36..421S - The Labyrinth of Star Formation, held in Greece, june 2012, Astrophysics and Space Science Proceedings, Volume 36. ISBN 978-3-319-03040-1. Springer International Publishing Switzerland, p. 421, 2014
bordeaux.peerReviewedoui
hal.identifierhal-00990055
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00990055v1
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