Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/27815
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Kong, Shuo | en_US |
dc.contributor.author | Tan, Jonathan C. | en_US |
dc.contributor.author | Caselli, Paola | en_US |
dc.contributor.author | FONTANI, FRANCESCO | en_US |
dc.contributor.author | Wang, Ke | en_US |
dc.contributor.author | Butler, Michael J. | en_US |
dc.date.accessioned | 2020-10-14T14:31:09Z | - |
dc.date.available | 2020-10-14T14:31:09Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 0004-637X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27815 | - |
dc.description.abstract | We present high-resolution (0.″2, 1000 au) 1.3 mm ALMA observations of the massive infrared dark cloud clump, G028.37+00.07-C1, thought to harbor the early stages of massive star formation. Using {{{N}}}<SUB>2</SUB>{{{D}}}<SUP>+</SUP>(3-2), we resolve the previously identified C1-S core, separating the bulk of its emission from two nearby protostellar sources. C1-S is thus identified as a massive (∼50 M <SUB>☉</SUB>), compact (∼0.1 pc diameter) starless core, e.g., with no signs of outflow activity. Being highly deuterated, this is a promising candidate for a pre-stellar core on the verge of collapse. An analysis of its dynamical state indicates a sub-virial velocity dispersion compared to a trans-Alfvénic turbulent core model. However, virial equilibrium could be achieved with sub-Alfvénic conditions involving magnetic field strengths of ∼2 mG. | en_US |
dc.language.iso | eng | en_US |
dc.title | Zooming in to Massive Star Birth | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/1538-4357/aae1b2 | en_US |
dc.identifier.scopus | 2-s2.0-85056663287 | en_US |
dc.identifier.isi | 000449168500010 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/1538-4357/aae1b2 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 867 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 94 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 6 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | THE ASTROPHYSICAL JOURNAL | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2018ApJ...867...94K | 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.orcid | 0000-0003-0348-3418 | - |
crisitem.journal.journalissn | 0004-637X | - |
crisitem.journal.ance | E016252 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
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File | Descrizione | Dimensioni | Formato | |
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1701.05953.pdf | postprint | 4.76 MB | Adobe PDF | Visualizza/apri |
Kong_2018_ApJ_867_94 compr.pdf | PDF editoriale | 2.77 MB | Adobe PDF | Visualizza/apri |
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