AGNs and their host galaxies in the local universe : two mass-independent Eddington ratio distribution functions characterize black hole growth.

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dc.contributor.authorWeigel, Anna
dc.contributor.authorEzequiel Treister
dc.contributor.authorSchawinski, Kevin
dc.contributor.authorCaplar, Neven
dc.contributor.authorWong, O. Ivy
dc.contributor.authorTrakhtenbrot, Benny
dc.date.accessioned2019-05-24T14:52:09Z
dc.date.available2019-05-24T14:52:09Z
dc.date.issued2017
dc.date.updated2019-05-17T15:36:53Z
dc.fuente.origenORCID
dc.identifier.doi10.3847/1538-4357/aa803b
dc.identifier.issn1538-4357
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/22794
dc.identifier.urihttps://doi.org/10.3847/1538-4357/aa803b
dc.identifier.wosidWOS:000408111400020
dc.issue.numeroNo. 2
dc.language.isoen
dc.nota.accesocontenido completo
dc.pagina.final33
dc.pagina.inicio1
dc.relation.isformatofThe Astrophysical Journal, vol. 845, no. 2 (Aug. 2017), 33 p.
dc.revistaThe Astrophysical Journales_ES
dc.rightsacceso abierto
dc.subjectGalaxieses_ES
dc.subjectEvolution - galaxieses_ES
dc.subjectLuminosity function, mass function - quasarses_ES
dc.subjectSupermasive black holeses_ES
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.titleAGNs and their host galaxies in the local universe : two mass-independent Eddington ratio distribution functions characterize black hole growth.es_ES
dc.typeartículo
dc.volumenVol. 845
sipa.codpersvinculados1031846
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