Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/27017
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Barišić, Ivana | en_US |
dc.contributor.author | VAN DER WEL, ARJEN | en_US |
dc.contributor.author | Bezanson, Rachel | en_US |
dc.contributor.author | Pacifici, Camilla | en_US |
dc.contributor.author | Noeske, Kai | en_US |
dc.contributor.author | Muñoz-Mateos, Juan C. | en_US |
dc.contributor.author | Franx, Marijn | en_US |
dc.contributor.author | Smolčić, Vernesa | en_US |
dc.contributor.author | Bell, Eric F. | en_US |
dc.contributor.author | Brammer, Gabriel | en_US |
dc.contributor.author | Calhau, João | en_US |
dc.contributor.author | Chauké, Priscilla | en_US |
dc.contributor.author | van Dokkum, Pieter G. | en_US |
dc.contributor.author | van Houdt, Josha | en_US |
dc.contributor.author | GALLAZZI, Anna Rita | en_US |
dc.contributor.author | Labbé, Ivo | en_US |
dc.contributor.author | Maseda, Michael V. | en_US |
dc.contributor.author | Muzzin, Adam | en_US |
dc.contributor.author | Sobral, David | en_US |
dc.contributor.author | Straatman, Caroline | en_US |
dc.contributor.author | Wu, Po-Feng | en_US |
dc.date.accessioned | 2020-09-01T08:16:26Z | - |
dc.date.available | 2020-09-01T08:16:26Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0004-637X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27017 | - |
dc.description.abstract | We investigate the stellar kinematics and stellar populations of 58 radio-loud galaxies of intermediate luminosities (L <SUB>3 GHz</SUB> > 10<SUP>23</SUP> W Hz<SUP>-1</SUP>) at 0.6 < z < 1. This sample is constructed by cross-matching galaxies from the deep VLT/VIMOS LEGA-C spectroscopic survey with the VLA 3 GHz data set. The LEGA-C continuum spectra reveal for the first time stellar velocity dispersions and age indicators of z ̃ 1 radio galaxies. We find that z ̃ 1 radio-loud active galactic nucleus (AGN) occur exclusively in predominantly old galaxies with high velocity dispersions: σ <SUB>*</SUB> > 175 km s<SUP>-1</SUP>, corresponding to black hole masses in excess of 10<SUP>8</SUP> M <SUB>☉</SUB>. Furthermore, we confirm that at a fixed stellar mass the fraction of radio-loud AGN at z ̃ 1 is five to 10 times higher than in the local universe, suggesting that quiescent, massive galaxies at z ̃ 1 switch on as radio AGN on average once every Gyr. Our results strengthen the existing evidence for a link between high black hole masses, radio loudness, and quiescence at z ̃ 1. | en_US |
dc.language.iso | eng | en_US |
dc.title | Stellar Dynamics and Star Formation Histories of z ̃ 1 Radio-loud Galaxies | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/1538-4357/aa8768 | en_US |
dc.identifier.scopus | 2-s2.0-85030150499 | en_US |
dc.identifier.isi | 000411574000011 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/1538-4357/aa8768 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 847 | en_US |
dc.relation.issue | 1 | en_US |
dc.relation.firstpage | 72 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | THE ASTROPHYSICAL JOURNAL | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2017ApJ...847...72B | 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.orcid | 0000-0002-9656-1800 | - |
crisitem.journal.journalissn | 0004-637X | - |
crisitem.journal.ance | E016252 | - |
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