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Characterising the high-mass star forming filament G351.776–0.527 with Herschel and APEX dust continuum and gas observations

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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