ALMA discovery of a rotating SO/SO$_2$ flow in HH212. A possible MHD disk wind?
dc.contributor.author | TABONE, B. | |
hal.structure.identifier | Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA] | |
dc.contributor.author | CABRIT, S. | |
dc.contributor.author | BIANCHI, E. | |
hal.structure.identifier | Génétique du cancer et des maladies neuropsychiatriques [GMFC] | |
dc.contributor.author | FERREIRA, Jorge | |
hal.structure.identifier | Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA] | |
dc.contributor.author | PINEAU DES FORÊTS, G. | |
hal.structure.identifier | Istituto Nazionale di Astrofisica [INAF] | |
dc.contributor.author | CODELLA, C. | |
hal.structure.identifier | Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA] | |
dc.contributor.author | GUSDORF, A. | |
hal.structure.identifier | Institut de RadioAstronomie Millimétrique [IRAM] | |
dc.contributor.author | GUETH, F. | |
hal.structure.identifier | INAF - Osservatorio Astrofisico di Arcetri [OAA] | |
dc.contributor.author | PODIO, L. | |
hal.structure.identifier | AMOR 2017 | |
dc.contributor.author | CHAPILLON, E. | |
dc.date.issued | 2017 | |
dc.identifier.issn | 0004-6361 | |
dc.description.abstractEn | We wish to put tight constraints on the possible contribution of an MHD disk wind (DW) to the HH212 molecular jet. We use ALMA Cycle 4 to map the inner outflow at $0.13" \sim$ 60~au resolution, and compare with synthetic predictions for DW models. We identify in SO/SO$_2$ a rotating flow wider and slower than the axial SiO jet. The broad outflow cavity seen in C$^{34}$S is not carved by a fast wide-angle wind but by this slower agent. Rotation signatures may be fitted by a DW of moderate lever arm launched out to $\sim$ 40 au, with SiO tracing dust-free streamlines from 0.05-0.3 au. If indeed a DW, it could limit the core-to-star efficiency to $\leq 50\%$. | |
dc.language.iso | en | |
dc.publisher | EDP Sciences | |
dc.subject.en | Astrophysics - Solar and Stellar Astrophysics | |
dc.subject.en | Astrophysics - Astrophysics of Galaxies | |
dc.subject.en | stars: formation | |
dc.subject.en | ISM: jets and outflows | |
dc.subject.en | ISM: individual objects: HH212 | |
dc.title.en | ALMA discovery of a rotating SO/SO$_2$ flow in HH212. A possible MHD disk wind? | |
dc.type | Article de revue | |
dc.identifier.doi | 10.1051/0004-6361/201731691 | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO] | |
dc.identifier.arxiv | 1710.01401 | |
bordeaux.journal | Astronomy and Astrophysics - A&A | |
bordeaux.peerReviewed | oui | |
hal.identifier | hal-01612954 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Internationale | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-01612954v1 | |
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