Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/27366
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Tabone, B. | en_US |
dc.contributor.author | Cabrit, S. | en_US |
dc.contributor.author | Bianchi, E. | en_US |
dc.contributor.author | Ferreira, J. | en_US |
dc.contributor.author | Pineau des Forêts, G. | en_US |
dc.contributor.author | CODELLA, CLAUDIO | en_US |
dc.contributor.author | Gusdorf, A. | en_US |
dc.contributor.author | Gueth, F. | en_US |
dc.contributor.author | PODIO, LINDA | en_US |
dc.contributor.author | Chapillon, E. | en_US |
dc.date.accessioned | 2020-09-14T14:49:41Z | - |
dc.date.available | 2020-09-14T14:49:41Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0004-6361 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27366 | - |
dc.description.abstract | We 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/SO<SUB>2</SUB>, a rotating flow that is wider and slower than the axial SiO jet. The broad outflow cavity seen in C<SUP>34</SUP>S 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%. | en_US |
dc.language.iso | eng | en_US |
dc.title | ALMA discovery of a rotating SO/SO2 flow in HH212. A possible MHD disk wind? | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1051/0004-6361/201731691 | en_US |
dc.identifier.scopus | 2-s2.0-85034420902 | en_US |
dc.identifier.isi | 000415265300001 | en_US |
dc.identifier.url | https://www.aanda.org/articles/aa/abs/2017/11/aa31691-17/aa31691-17.html | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 607 | en_US |
dc.relation.firstpage | L6 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | ASTRONOMY & ASTROPHYSICS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2017A&A...607L...6T | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.orcid | 0000-0003-1514-3074 | - |
crisitem.author.orcid | 0000-0003-2733-5372 | - |
crisitem.journal.journalissn | 0004-6361 | - |
crisitem.journal.ance | E016240 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
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File | Descrizione | Dimensioni | Formato | |
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aa31691-17.pdf | PDF editoriale | 1.51 MB | Adobe PDF | Visualizza/apri |
1710.01401.pdf | postprint | 2.28 MB | Adobe PDF | Visualizza/apri |
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