Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/29820
DC Field | Value | Language |
---|---|---|
dc.contributor.author | GOVONI, FEDERICA | en_US |
dc.contributor.author | Orrù, E. | en_US |
dc.contributor.author | BONAFEDE, ANNALISA | en_US |
dc.contributor.author | Iacobelli, M. | en_US |
dc.contributor.author | Paladino, Rosita | en_US |
dc.contributor.author | VAZZA, FRANCO | en_US |
dc.contributor.author | MURGIA, MATTEO | en_US |
dc.contributor.author | VACCA, VALENTINA | en_US |
dc.contributor.author | Giovannini, Gabriele | en_US |
dc.contributor.author | Feretti, L. | en_US |
dc.contributor.author | Loi, F. | en_US |
dc.contributor.author | BERNARDI, GIANNI | en_US |
dc.contributor.author | Ferrari, C. | en_US |
dc.contributor.author | Pizzo, R. F. | en_US |
dc.contributor.author | Gheller, C. | en_US |
dc.contributor.author | Manti, S. | en_US |
dc.contributor.author | Brüggen, M. | en_US |
dc.contributor.author | BRUNETTI, GIANFRANCO | en_US |
dc.contributor.author | CASSANO, Rossella | en_US |
dc.contributor.author | de Gasperin, F. | en_US |
dc.contributor.author | Enßlin, T. A. | en_US |
dc.contributor.author | Hoeft, M. | en_US |
dc.contributor.author | Horellou, C. | en_US |
dc.contributor.author | Junklewitz, H. | en_US |
dc.contributor.author | Röttgering, H. J. A. | en_US |
dc.contributor.author | Scaife, A. M. M. | en_US |
dc.contributor.author | Shimwell, T. W. | en_US |
dc.contributor.author | van Weeren, R. J. | en_US |
dc.contributor.author | Wise, M. | en_US |
dc.date.accessioned | 2021-01-18T14:13:53Z | - |
dc.date.available | 2021-01-18T14:13:53Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.issn | 0036-8075 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/29820 | - |
dc.description.abstract | Galaxy clusters are the most massive gravitationally bound structures in the Universe. They grow by accreting smaller structures in a merging process that produces shocks and turbulence in the intracluster gas. We observed a ridge of radio emission connecting the merging galaxy clusters Abell 0399 and Abell 0401 with the Low-Frequency Array (LOFAR) telescope network at 140 megahertz. This emission requires a population of relativistic electrons and a magnetic field located in a filament between the two galaxy clusters. We performed simulations to show that a volume-filling distribution of weak shocks may reaccelerate a preexisting population of relativistic particles, producing emission at radio wavelengths that illuminates the magnetic ridge. | en_US |
dc.language.iso | eng | en_US |
dc.title | A radio ridge connecting two galaxy clusters in a filament of the cosmic web | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1126/science.aat7500 | en_US |
dc.identifier.scopus | 2-s2.0-85067439923 | en_US |
dc.identifier.isi | 000471079600005 | en_US |
dc.identifier.url | https://science.sciencemag.org/content/364/6444/981 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 364 | en_US |
dc.relation.issue | 6444 | en_US |
dc.relation.firstpage | 981 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | SCIENCE | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2019Sci...364..981G | 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 |
local.message.claim | 2021-01-19T09:25:39.384+0100|||rp08088|||submit_approve|||dc_contributor_author|||None | * |
item.grantfulltext | open | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
item.cerifentitytype | Publications | - |
crisitem.journal.journalissn | 0036-8075 | - |
crisitem.journal.ance | E151981 | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.orcid | 0000-0003-3644-3084 | - |
crisitem.author.orcid | 0000-0002-5068-4581 | - |
crisitem.author.orcid | 0000-0001-9143-6026 | - |
crisitem.author.orcid | 0000-0002-2821-7928 | - |
crisitem.author.orcid | 0000-0002-4800-0806 | - |
crisitem.author.orcid | 0000-0003-1997-0771 | - |
crisitem.author.orcid | 0000-0003-4916-6362 | - |
crisitem.author.orcid | 0000-0002-0916-7443 | - |
crisitem.author.orcid | 0000-0003-4195-8613 | - |
crisitem.author.orcid | 0000-0003-4046-0637 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Science1906.07584.pdf | preprint | 4.76 MB | Adobe PDF | View/Open |
Govoni_2019.pdf | [Administrators only] | 1.05 MB | Adobe PDF |
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