Determining the radio active galactic nuclei contribution to the radio-far-infrared correlation using the black hole Fundamental Plane relation

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dc.contributor.authorWong, O.
dc.contributor.authorKoss, M.
dc.contributor.authorSchawinski, K.
dc.contributor.authorKapinska, A.
dc.contributor.authorLamperti, I.
dc.contributor.authorOh, K.
dc.contributor.authorRicci, Claudio
dc.contributor.authorBerney, S.
dc.contributor.authorTrakhtenbrot, B.
dc.date.accessioned2021-05-13T17:51:27Z
dc.date.available2021-05-13T17:51:27Z
dc.date.issued2016
dc.fuente.origenConveris
dc.identifier.doi10.1093/mnras/stw957
dc.identifier.eissn1365-2966
dc.identifier.issn0035-8711
dc.identifier.urihttps://doi.org/10.1093/mnras/stw957
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/58348
dc.identifier.wosidWOS:000379832800034
dc.issue.numeroNo. 2
dc.language.isoen
dc.pagina.final1597
dc.pagina.inicio1588
dc.revistaMonthly Notices of the Royal Astronomical Societyes_ES
dc.rightsacceso restringido
dc.titleDetermining the radio active galactic nuclei contribution to the radio-far-infrared correlation using the black hole Fundamental Plane relationes_ES
dc.typeartículo
dc.volumenVol. 460
sipa.codpersvinculados1015217
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