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http://hdl.handle.net/20.500.12386/27491
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | D'AMMANDO, FILIPPO | en_US |
dc.contributor.author | Acosta-Pulido, J. A. | en_US |
dc.contributor.author | CAPETTI, Alessandro | en_US |
dc.contributor.author | BALDI, RANIERI DIEGO | en_US |
dc.contributor.author | ORIENTI, Monica | en_US |
dc.contributor.author | RAITERI, Claudia Maria | en_US |
dc.contributor.author | Ramos Almeida, C. | en_US |
dc.date.accessioned | 2020-09-28T12:40:01Z | - |
dc.date.available | 2020-09-28T12:40:01Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27491 | - |
dc.description.abstract | The detection of γ-ray emission from narrow-line Seyfert 1 galaxies (NLSy1) has challenged the idea that large black hole (BH) masses (≥10<SUP>8</SUP> M<SUB>☉</SUB>) are needed to launch relativistic jets. We present near-infrared imaging data of the γ-ray-emitting NLSy1 PKS 1502+036 obtained with the Very Large Telescope. Its surface brightness profile, extending to ∼20 kpc, is well described by the combination of a nuclear component and a bulge with a Sérsic index n = 3.5, which is indicative of an elliptical galaxy. A circumnuclear structure observed near PKS 1502+036 may be the result of galaxy interactions. A BH mass of ∼7 × 10<SUP>8</SUP> M<SUB>☉</SUB> has been estimated by the bulge luminosity. The presence of an additional faint disc component cannot be ruled out with the present data, but this would reduce the BH mass estimate by only ∼30 per cent. These results, together with analogous findings obtained for FBQS J1644+2619, indicate that the relativistic jets in γ-ray-emitting NLSy1 are likely produced by massive black holes at the centre of elliptical galaxies. | en_US |
dc.language.iso | eng | en_US |
dc.title | The host galaxy of the γ-ray-emitting narrow-line Seyfert 1 galaxy PKS 1502+036 | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnrasl/sly072 | en_US |
dc.identifier.scopus | 2-s2.0-85048866588 | en_US |
dc.identifier.isi | 000450777200013 | en_US |
dc.identifier.url | https://academic.oup.com/mnrasl/article/478/1/L66/4987211 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 478 | en_US |
dc.relation.issue | 1 | en_US |
dc.relation.firstpage | L66 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 7 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | ESP | 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.478L..66D | 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 | O.A. Torino | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | O.A. Torino | - |
crisitem.author.orcid | 0000-0001-7618-7527 | - |
crisitem.author.orcid | 0000-0003-3684-4275 | - |
crisitem.author.orcid | 0000-0002-1824-0411 | - |
crisitem.author.orcid | 0000-0003-4470-7094 | - |
crisitem.author.orcid | 0000-0003-1784-2784 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
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File | Descrizione | Dimensioni | Formato | |
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sly072.pdf | Pdf editoriale | 3.74 MB | Adobe PDF | Visualizza/apri |
1804.10220.pdf | postprint | 1.26 MB | Adobe PDF | Visualizza/apri |
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