Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/29605
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Ursini, Francesco | en_US |
dc.contributor.author | Petrucci, P. -O. | en_US |
dc.contributor.author | Matt, G. | en_US |
dc.contributor.author | BIANCHI, SIMONE | en_US |
dc.contributor.author | CAPPI, MASSIMO | en_US |
dc.contributor.author | DADINA, MAURO | en_US |
dc.contributor.author | GRANDI, PAOLA | en_US |
dc.contributor.author | TORRESI, ELEONORA | en_US |
dc.contributor.author | Ballantyne, D. R. | en_US |
dc.contributor.author | De Marco, B. | en_US |
dc.contributor.author | DE ROSA, ADRIANO GIUSEPPE | en_US |
dc.contributor.author | GIROLETTI, MARCELLO | en_US |
dc.contributor.author | Malzac, J. | en_US |
dc.contributor.author | Marinucci, A. | en_US |
dc.contributor.author | Middei, R. | en_US |
dc.contributor.author | PONTI, GABRIELE | en_US |
dc.contributor.author | TORTOSA, ALESSIA | en_US |
dc.date.accessioned | 2021-01-08T10:46:41Z | - |
dc.date.available | 2021-01-08T10:46:41Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/29605 | - |
dc.description.abstract | We present the analysis of five joint XMM-Newton/NuSTAR observations, 20 ks each and separated by 12 days, of the broad-line radio galaxy 3C 382. The data were obtained as part of a campaign performed in September-October 2016 simultaneously with Very Long Baseline Array. The radio data and their relation with the X-ray ones will be discussed in a following paper. The source exhibits a moderate flux variability in the UV/X-ray bands, and a limited spectral variability especially in the soft X-ray band. In agreement with past observations, we find the presence of a warm absorber, an iron Kα line with no associated Compton reflection hump, and a variable soft excess well described by a thermal Comptonization component. The data are consistent with a `two-corona' scenario, in which the UV emission and soft excess are produced by a warm (kT ≃ 0.6 keV), optically thick (τ ≃ 20) corona consistent with being a slab fully covering a nearly passive accretion disc, while the hard X-ray emission is due to a hot corona intercepting roughly 10 per cent of the soft emission. These results are remarkably similar to those generally found in radio-quiet Seyferts, thus suggesting a common accretion mechanism. | en_US |
dc.language.iso | eng | en_US |
dc.title | Radio/X-ray monitoring of the broad-line radio galaxy 3C 382. High-energy view with XMM-Newton and NuSTAR | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/sty1258 | en_US |
dc.identifier.scopus | 2-s2.0-85052466594 | en_US |
dc.identifier.isi | 000439547400092 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article-abstract/478/2/2663/4996367 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/pdf-lookup/doi/10.1093/mnras/sty1258 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 478 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 2663 | en_US |
dc.relation.lastpage | 2675 | en_US |
dc.type.referee | REF_1 | 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 | 2018MNRAS.478.2663U | 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::PE9_6 Stars and stellar systems | 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 | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.orcid | 0000-0001-9442-7897 | - |
crisitem.author.orcid | 0000-0001-6966-8920 | - |
crisitem.author.orcid | 0000-0002-7858-7564 | - |
crisitem.author.orcid | 0000-0003-1848-6013 | - |
crisitem.author.orcid | 0000-0002-5201-010X | - |
crisitem.author.orcid | 0000-0002-8657-8852 | - |
crisitem.author.orcid | 0000-0003-0293-3608 | - |
crisitem.author.orcid | 0000-0003-3450-6483 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
Appears in Collections: | 1.01 Articoli in rivista |
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File | Description | Size | Format | |
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sty1258.pdf | PDF editoriale | 1.35 MB | Adobe PDF | View/Open |
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