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LEGO – II. A 3 mm molecular line study covering 100 pc of one of the most actively star-forming portions within the Milky Way disc

dc.contributor.authorBARNES, A
dc.contributor.authorKAUFFMANN, J
dc.contributor.authorBIGIEL, F
dc.contributor.authorBRINKMANN, N
dc.contributor.authorCOLOMBO, D
dc.contributor.authorGUZMÁN, A
dc.contributor.authorKIM, W
dc.contributor.authorSZŰCS, L
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorWAKELAM, V
dc.contributor.authorAALTO, S
dc.contributor.authorALBERTSSON, T
dc.contributor.authorEVANS, N
dc.contributor.authorGLOVER, S
dc.contributor.authorGOLDSMITH, P
dc.contributor.authorKRAMER, C
dc.contributor.authorMENTEN, K
dc.contributor.authorNISHIMURA, Y
dc.contributor.authorVITI, S
dc.contributor.authorWATANABE, Y
dc.contributor.authorWEISS, A
dc.contributor.authorWIENEN, M
dc.contributor.authorWIESEMEYER, H
dc.contributor.authorWYROWSKI, F
dc.date.issued2020-09-11
dc.identifier.issn0035-8711
dc.language.isoen
dc.publisherOxford University Press (OUP): Policy P - Oxford Open Option A
dc.title.enLEGO – II. A 3 mm molecular line study covering 100 pc of one of the most actively star-forming portions within the Milky Way disc
dc.typeArticle de revue
dc.identifier.doi10.1093/mnras/staa1814
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]
dc.identifier.arxiv2007.11005
bordeaux.journalMonthly Notices of the Royal Astronomical Society
bordeaux.page1972-2001
bordeaux.volume497
bordeaux.issue2
bordeaux.peerReviewedoui
hal.identifierhal-03007581
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-03007581v1
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