Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/29482
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Del Zanna, L. | en_US |
dc.contributor.author | Olmi, Barbara | en_US |
dc.contributor.author | AMATO, Elena | en_US |
dc.contributor.author | BUCCIANTINI, NICCOLO' | en_US |
dc.contributor.author | Mignone, A. | en_US |
dc.date.accessioned | 2021-01-05T11:23:17Z | - |
dc.date.available | 2021-01-05T11:23:17Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.issn | 2037-4631 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/29482 | - |
dc.description.abstract | Pulsar wind nebulae inside young supernova remnants, and in particular the Crab nebula, are probably the best laboratories for high-energy astrophysics and relativistic plasma physics. They have been modeled numerically for more than a decade through multi-dimensional relativistic MHD simulations, relying on axial symmetry until a few years ago while currently using full three-dimensional simulations employing adaptive meshes. Here, we discuss the most recent findings, especially those obtained by our Arcetri group, focusing on the problem of magnetic field dissipation inside the nebula. | en_US |
dc.language.iso | eng | en_US |
dc.title | The Crab nebula in the light of three-dimensional relativistic MHD simulations | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1007/s12210-019-00759-y | en_US |
dc.identifier.scopus | 2-s2.0-85059878602 | en_US |
dc.identifier.isi | 000501308500012 | en_US |
dc.identifier.url | https://link.springer.com/article/10.1007/s12210-019-00759-y | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 30 | en_US |
dc.relation.issue | S1 | en_US |
dc.relation.firstpage | 93 | en_US |
dc.relation.lastpage | 96 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 5 | en_US |
dc.description.international | no | en_US |
dc.contributor.country | ITA | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | RENDICONTI LINCEI. SCIENZE FISICHE E NATURALI | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | https://ui.adsabs.harvard.edu/abs/2019RLSFN.tmp....1D/abstract | 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.dept | O.A. Arcetri | - |
crisitem.author.orcid | 0000-0001-6022-8216 | - |
crisitem.author.orcid | 0000-0002-9881-8112 | - |
crisitem.author.orcid | 0000-0002-8848-1392 | - |
crisitem.journal.journalissn | 2037-4631 | - |
crisitem.journal.ance | E202946 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
LdZ_Lincei.pdf | postprint | 876.38 kB | Adobe PDF | View/Open |
DelZanna2019_Article_TheCrabNebulaInTheLightOfThree.pdf | [Administrators only] | 881.58 kB | Adobe PDF |
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