DC FieldValueLanguage
dc.contributor.authorMićić, Miroslaven
dc.contributor.authorMartinović, Nemanjaen
dc.date.accessioned2020-05-01T20:12:37Z-
dc.date.available2020-05-01T20:12:37Z-
dc.date.issued2014-01-01en
dc.identifier.isbn978-8-680-01980-2en
dc.identifier.urihttp://researchrepository.mi.sanu.ac.rs/handle/123456789/1039-
dc.description.abstractWe use high resolution cosmological numerical simulation to identify AGNs in field massive galaxies in redshift range z=[0.8, 2.5]. Assuming that their activity is merger driven and that the final product of their accretion is an M-σ SMBH, we calculate expected AGN luminosity at the peak accretion activity. We compare these luminosities to those observed in AGNs of the COSMOS survey and find that most of the observed AGNs have passed their peak activity, accreting at lower Eddington ratios. This explains why a large number of AGNs is observed in red sequence galaxies.en
dc.publisherAstronomical Observatory-
dc.relation.ispartofProceedings of the XVII National Conference of Astronomers of Serbiaen
dc.titleAgn phase: Matching numerical simulations to observationsen
dc.typeConference Paperen
dc.relation.conference17th National Conference of Astronomers of Serbia; Ceremonial Hall in Belgrade University Building Belgrade; Serbia; 23 September 2014 through 27 September 2014-
dc.identifier.scopus2-s2.0-85040656010en
dc.relation.firstpage263en
dc.relation.lastpage268en
item.cerifentitytypePublications-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
item.openairetypeConference Paper-
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