Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/29265
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Smirnova-Pinchukova, I. | en_US |
dc.contributor.author | Husemann, B. | en_US |
dc.contributor.author | Busch, G. | en_US |
dc.contributor.author | Appleton, P. | en_US |
dc.contributor.author | Bethermin, M. | en_US |
dc.contributor.author | Combes, F. | en_US |
dc.contributor.author | Croom, S. | en_US |
dc.contributor.author | Davis, T. A. | en_US |
dc.contributor.author | Fischer, C. | en_US |
dc.contributor.author | GASPARI, MASSIMO | en_US |
dc.contributor.author | Groves, B. | en_US |
dc.contributor.author | Klein, R. | en_US |
dc.contributor.author | O'Dea, C. P. | en_US |
dc.contributor.author | Pérez-Torres, M. | en_US |
dc.contributor.author | Scharwächter, J. | en_US |
dc.contributor.author | Singha, M. | en_US |
dc.contributor.author | Tremblay, G. R. | en_US |
dc.contributor.author | Urrutia, T. | en_US |
dc.date.accessioned | 2020-12-29T10:49:44Z | - |
dc.date.available | 2020-12-29T10:49:44Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.issn | 0004-6361 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/29265 | - |
dc.description.abstract | The [C II]λ158 μm line is one of the strongest far-infrared (FIR) lines and an important coolant in the interstellar medium of galaxies that is accessible out to high redshifts. The excitation of [C II] is complex and can best be studied in detail at low redshifts. Here we report the discovery of the highest global [C II] excess with respect to the FIR luminosity in the nearby AGN host galaxy HE 1353-1917. This galaxy is exceptional among a sample of five targets because the AGN ionization cone and radio jet directly intercept the cold galactic disk. As a consequence, a massive multiphase gas outflow on kiloparsec scales is embedded in an extended narrow-line region. Because HE 1353-1917 is distinguished by these special properties from our four bright AGN, we propose that a global [C II] excess in AGN host galaxies could be a direct signature of a multiphase AGN-driven outflow with a high mass-loading factor. | en_US |
dc.language.iso | eng | en_US |
dc.title | The Close AGN Reference Survey (CARS): Discovery of a global [C II] 158 μm line excess in AGN HE 1353-1917 | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1051/0004-6361/201935577 | en_US |
dc.identifier.scopus | 2-s2.0-85082833842 | en_US |
dc.identifier.isi | 000471640400001 | en_US |
dc.identifier.url | https://www.aanda.org/articles/aa/abs/2019/06/aa35577-19/aa35577-19.html | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 626 | en_US |
dc.relation.firstpage | L3 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | ASTRONOMY & ASTROPHYSICS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2019A&A...626L...3S | 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.orcid | 0000-0003-2754-9258 | - |
crisitem.journal.journalissn | 0004-6361 | - |
crisitem.journal.ance | E016240 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
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aa35577-19.pdf | Pdf editoriale | 9.43 MB | Adobe PDF | Visualizza/apri |
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