Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/32514
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Revet, Guilhem | en_US |
dc.contributor.author | Chen, Sophia N. | en_US |
dc.contributor.author | Bonito, Rosaria | en_US |
dc.contributor.author | Khiar, Benjamin | en_US |
dc.contributor.author | Filippov, Evgeny | en_US |
dc.contributor.author | Argiroffi, Costanza | en_US |
dc.contributor.author | Higginson, Drew P. | en_US |
dc.contributor.author | ORLANDO, Salvatore | en_US |
dc.contributor.author | Béard, Jérôme | en_US |
dc.contributor.author | Blecher, Marius | en_US |
dc.contributor.author | Borghesi, Marco | en_US |
dc.contributor.author | Burdonov, Konstantin | en_US |
dc.contributor.author | Khaghani, Dimitri | en_US |
dc.contributor.author | Naughton, Kealan | en_US |
dc.contributor.author | Pépin, Henri | en_US |
dc.contributor.author | Portugall, Oliver | en_US |
dc.contributor.author | Riquier, Raphael | en_US |
dc.contributor.author | Rodriguez, Rafael | en_US |
dc.contributor.author | Ryazantsev, Sergei N. | en_US |
dc.contributor.author | Yu. Skobelev, Igor | en_US |
dc.contributor.author | Soloviev, Alexander | en_US |
dc.contributor.author | Willi, Oswald | en_US |
dc.contributor.author | Pikuz, Sergey | en_US |
dc.contributor.author | Ciardi, Andrea | en_US |
dc.contributor.author | Fuchs, Julien | en_US |
dc.date.accessioned | 2022-07-15T15:45:46Z | - |
dc.date.available | 2022-07-15T15:45:46Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 2375-2548 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/32514 | - |
dc.description.abstract | Accretion dynamics in the forming of young stars is still object of debate because of limitations in observations and modelling. Through scaled laboratory experiments of collimated plasma accretion onto a solid in the presence of a magnetic field, we open first window on this phenomenon by tracking, with spatial and temporal resolution, the dynamics of the system and simultaneously measuring multiband emissions. We observe in these experiments that matter, upon impact, is laterally ejected from the solid surface, then refocused by the magnetic field toward the incoming stream. Such ejected matter forms a plasma shell that envelops the shocked core, reducing escaped X-ray emission. This demonstrates one possible structure reconciling current discrepancies between mass accretion rates derived from X-ray and optical observations. | en_US |
dc.language.iso | eng | en_US |
dc.title | Laboratory unraveling of matter accretion in young stars | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1126/sciadv.1700982 | en_US |
dc.identifier.url | https://advances.sciencemag.org/content/3/11/e1700982 | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 3 | en_US |
dc.relation.issue | 11 | en_US |
dc.relation.firstpage | e1700982 | en_US |
dc.relation.article | e1700982 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 25 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | GBR | en_US |
dc.contributor.country | FRA | en_US |
dc.contributor.country | DEU | en_US |
dc.contributor.country | ESP | en_US |
dc.contributor.country | CAN | en_US |
dc.contributor.country | RUS | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | SCIENCE ADVANCES | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_4 Formation of stars and planets | 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. Palermo | - |
crisitem.author.dept | O.A. Palermo | - |
crisitem.author.dept | O.A. Palermo | - |
crisitem.author.orcid | 0000-0001-9297-7748 | - |
crisitem.author.orcid | 0000-0003-2073-1348 | - |
crisitem.author.orcid | 0000-0003-2836-540X | - |
crisitem.journal.journalissn | 2375-2548 | - |
crisitem.journal.ance | E231702 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
e1700982.full.pdf | PDF editoriale | 630.02 kB | Adobe PDF | View/Open |
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Items in DSpace are published in Open Access, unless otherwise indicated.