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dc.contributor.authorLEURINI, S.
dc.contributor.authorSCHISANO, E.
dc.contributor.authorPILLAI, T.
dc.contributor.authorGIANNETTI, A.
dc.contributor.authorURQUHART, J.
hal.structure.identifierFORMATION STELLAIRE 2020
dc.contributor.authorCSENGERI, T.
dc.contributor.authorCASU, S.
dc.contributor.authorCUNNINGHAM, M.
dc.contributor.authorELIA, D.
dc.contributor.authorJONES, P.
dc.contributor.authorKÖNIG, C.
dc.contributor.authorMOLINARI, S.
dc.contributor.authorSTANKE, T.
dc.contributor.authorTESTI, L.
dc.contributor.authorWYROWSKI, F.
dc.contributor.authorMENTEN, K.
dc.date.issued2019-01
dc.identifier.issn0004-6361
dc.language.isoen
dc.publisherEDP Sciences
dc.title.enCharacterising the high-mass star forming filament G351.776–0.527 with Herschel and APEX dust continuum and gas observations
dc.typeArticle de revue
dc.identifier.doi10.1051/0004-6361/201833612
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]
dc.identifier.arxiv1812.01035
bordeaux.journalAstronomy and Astrophysics - A&A
bordeaux.pageA130
bordeaux.volume621
bordeaux.peerReviewedoui
hal.identifierhal-03054130
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-03054130v1
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