Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/28406
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Liu, Teng | en_US |
dc.contributor.author | Merloni, Andrea | en_US |
dc.contributor.author | Wang, Jun-Xian | en_US |
dc.contributor.author | TOZZI, Paolo | en_US |
dc.contributor.author | Shen, Yue | en_US |
dc.contributor.author | Brusa, Marcella | en_US |
dc.contributor.author | Salvato, Mara | en_US |
dc.contributor.author | Nandra, Kirpal | en_US |
dc.contributor.author | Comparat, Johan | en_US |
dc.contributor.author | Liu, Zhu | en_US |
dc.contributor.author | PONTI, GABRIELE | en_US |
dc.contributor.author | Coffey, Damien | en_US |
dc.date.accessioned | 2020-11-17T18:01:55Z | - |
dc.date.available | 2020-11-17T18:01:55Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/28406 | - |
dc.description.abstract | Using the X-ray-selected active galactic nuclei (AGN) from the XMM-XXL north survey and the Sloan Digital Sky Survey-Baryon Oscillation Spectroscopic Survey spectroscopic follow-up of them, we compare the properties of X-ray unobscured and obscured broad-line AGN (BLAGN1 and BLAGN2; N<SUB>H</SUB> below and above 10<SUP>21.5</SUP> cm<SUP>-2</SUP>), including their X-ray luminosity L<SUB>X</SUB>, black hole mass, Eddington ratio λ<SUB>Edd</SUB>, optical continuum, and line features. We find that BLAGN2 have systematically larger broad line widths and hence apparently higher (lower) M<SUB>BH</SUB> (λ<SUB>Edd</SUB>) than BLAGN1. We also find that the X-ray obscuration in BLAGN tends to coincide with optical dust extinction, which is optically thinner than that in narrow-line AGN (NLAGN) and likely partial covering to the broad-line region. All the results can be explained in the framework of a multicomponent, clumpy torus model by interpreting BLAGN2 as an intermediate type between BLAGN1 and NLAGN in terms of an intermediate inclination angle. <P /> | en_US |
dc.language.iso | eng | en_US |
dc.title | Probing AGN inner structure with X-ray obscured type 1 AGN | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/sty1751 | en_US |
dc.identifier.scopus | 2-s2.0-85051564829 | en_US |
dc.identifier.isi | 000441383700055 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article-abstract/479/4/5022/5049307 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 479 | en_US |
dc.relation.issue | 4 | en_US |
dc.relation.firstpage | 5022 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 12 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | DEU | 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.479.5022L | 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 | O.A. Arcetri | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.orcid | 0000-0003-3096-9966 | - |
crisitem.author.orcid | 0000-0003-0293-3608 | - |
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 | |
---|---|---|---|---|
sty1751.pdf | PDF editoriale | 3.09 MB | Adobe PDF | View/Open |
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