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hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA]
dc.contributor.authorTABONE, B.
hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA]
dc.contributor.authorCABRIT, S.
dc.contributor.authorBIANCHI, E.
dc.contributor.authorFERREIRA, J.
hal.structure.identifierInstitut d'astrophysique spatiale [IAS]
hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA]
dc.contributor.authorPINEAU DES FORÊTS, G.
dc.contributor.authorCODELLA, C.
hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA]
dc.contributor.authorGUSDORF, A.
hal.structure.identifierInstitut de RadioAstronomie Millimétrique [IRAM]
dc.contributor.authorGUETH, F.
hal.structure.identifierINAF - Osservatorio Astrofisico di Arcetri [OAA]
dc.contributor.authorPODIO, L.
hal.structure.identifierAMOR 2017
dc.contributor.authorCHAPILLON, E.
dc.date.issued2017-11
dc.identifier.issn0004-6361
dc.description.abstractEnWe wish to constrain the possible contribution of a magnetohydrodynamic disk wind (DW) to the HH212 molecular jet. We mapped the flow base with ALMA Cycle 4 at 0.̋13 ~ 60 au resolution and compared these observations with synthetic DW predictions. We identified, in SO/SO2, a rotating flow that is wider and slower than the axial SiO jet. The broad outflow cavity seen in C34S is not carved by a fast wide-angle wind but by this slower agent. Rotation signatures may be fitted by a DW of a moderate lever arm launched out to ~40 au with SiO tracing dust-free streamlines from 0.05−0.3 au. Such a DW could limit the core-to-star efficiency to ≤50%.
dc.language.isoen
dc.publisherEDP Sciences
dc.subject.enstars: formation
dc.subject.enISM: jets and outflows
dc.subject.enISM: individual objects: HH212
dc.title.enALMA discovery of a rotating SO/SO2 flow in HH212
dc.title.enA possible MHD disk wind?
dc.typeArticle de revue
dc.identifier.doi10.1051/0004-6361/201731691
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
bordeaux.journalAstronomy and Astrophysics - A&A
bordeaux.pageL6
bordeaux.volume607
bordeaux.peerReviewedoui
hal.identifierhal-02238172
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-02238172v1
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