Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/27312
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Brown, S. | en_US |
dc.contributor.author | Vernstrom, T. | en_US |
dc.contributor.author | CARRETTI, ETTORE | en_US |
dc.contributor.author | Dolag, K. | en_US |
dc.contributor.author | Gaensler, B. M. | en_US |
dc.contributor.author | Staveley-Smith, L. | en_US |
dc.contributor.author | BERNARDI, GIANNI | en_US |
dc.contributor.author | Haverkorn, M. | en_US |
dc.contributor.author | Kesteven, M. | en_US |
dc.contributor.author | POPPI, Sergio | en_US |
dc.date.accessioned | 2020-09-11T10:30:35Z | - |
dc.date.available | 2020-09-11T10:30:35Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27312 | - |
dc.description.abstract | We set limits on the presence of the synchrotron cosmic web through the cross-correlation of the 2.3 GHz S-PASS survey with a model of the local cosmic web derived from constrained magnetohydrodynamic (MHD) simulations. The MHD simulation assumes cosmologically seeded magnetic fields amplified during large-scale structure formation and a population of relativistic electrons/positrons from proton-proton collisions within the intergalactic medium. We set a model-dependent 3σ upper limit on the synchrotron surface brightness of 0.16 mJy arcmin<SUP>-2</SUP> at 2.3 GHz in filaments. Extrapolating from magnetic field maps created from the simulation, we infer an upper limit (density-weighted) magnetic field of 0.03 (0.13) μG in filaments at the current epoch and a limit on the primordial magnetic field (PMF) of B<SUB>PMF</SUB> < 1.0 nG. | en_US |
dc.language.iso | eng | en_US |
dc.title | Limiting magnetic fields in the cosmic web with diffuse radio emission | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stx746 | en_US |
dc.identifier.scopus | 2-s2.0-85032010670 | en_US |
dc.identifier.isi | 000402819700037 | en_US |
dc.identifier.url | http://arxiv.org/abs/1703.07829v1 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/468/4/4246/3091005 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 468 | en_US |
dc.relation.issue | 4 | en_US |
dc.relation.firstpage | 4246 | en_US |
dc.relation.lastpage | 4253 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | AUS | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2017MNRAS.468.4246B | en_US |
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 | 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 | IRA Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.orcid | 0000-0002-3973-8403 | - |
crisitem.author.orcid | 0000-0002-0916-7443 | - |
crisitem.author.orcid | 0000-0002-4698-2607 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
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