Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/30732
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Ursini, Francesco | en_US |
dc.contributor.author | BASSANI, LOREDANA | en_US |
dc.contributor.author | PANESSA, Francesca | en_US |
dc.contributor.author | BAZZANO, ANGELA | en_US |
dc.contributor.author | Bird, A. J. | en_US |
dc.contributor.author | MALIZIA, ANGELA | en_US |
dc.contributor.author | Ubertini, P. | en_US |
dc.date.accessioned | 2021-04-12T09:32:21Z | - |
dc.date.available | 2021-04-12T09:32:21Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/30732 | - |
dc.description.abstract | We present a broad-band X-ray spectral analysis of the radio-loud active galactic nuclei NGC 612, 4C 73.08 and 3C 452, exploiting archival data from NuSTAR, XMM-Newton, Swift and INTEGRAL. These Compton-thick candidates are the most absorbed sources among the hard X-ray selected radio galaxies studied in Panessa et al. We find an X-ray absorbing column density in every case below 1.5 × 10<SUP>24</SUP> cm<SUP>-2</SUP>, and no evidence for a strong reflection continuum or iron K α line. Therefore, none of these sources is properly Compton-thick. We review other Compton-thick radio galaxies reported in the literature, arguing that we currently lack strong evidences for heavily absorbed radio-loud AGNs. | en_US |
dc.language.iso | eng | en_US |
dc.title | Where are Compton-thick radio galaxies? A hard X-ray view of three candidates | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stx3159 | en_US |
dc.identifier.scopus | 2-s2.0-85045895439 | en_US |
dc.identifier.isi | 000424977800100 | en_US |
dc.identifier.url | http://arxiv.org/abs/1712.01300v1 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/474/4/5684/4712227 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 474 | en_US |
dc.relation.issue | 4 | en_US |
dc.relation.firstpage | 5684 | en_US |
dc.relation.lastpage | 5693 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 7 | 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 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2018MNRAS.474.5684U | 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 | IAPS Roma | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0001-9442-7897 | - |
crisitem.author.orcid | 0000-0003-4858-6963 | - |
crisitem.author.orcid | 0000-0003-0543-3617 | - |
crisitem.author.orcid | 0000-0002-2017-4396 | - |
crisitem.author.orcid | 0000-0002-6558-1163 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
1712.01300.pdf | postprint | 795.3 kB | Adobe PDF | View/Open |
stx3159.pdf | Pdf editoriale | 1.17 MB | Adobe PDF | View/Open |
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