The dependence of mass and environment on the secular processes of AGNs in terms of morphology, colour, and specific star-formation rate

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dc.contributor.authorArgudo-Fernandez, M.
dc.contributor.authorLacerna Zambrano, Iván Andrés
dc.contributor.authorDuarte Puertas, S.
dc.date.accessioned2021-05-31T03:43:21Z
dc.date.available2021-05-31T03:43:21Z
dc.date.issued2018
dc.fechaingreso.objetodigital2024-08-14
dc.format.extent13 páginas
dc.fuente.origenConveris
dc.identifier.doi10.1051/0004-6361/201833328
dc.identifier.issn0004-6361
dc.identifier.urihttps://doi.org/10.1051/0004-6361/201833328
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/59798
dc.identifier.wosidWOS:000452472000002
dc.language.isoen
dc.nota.accesoContenido completo
dc.pagina.final13
dc.pagina.inicio1
dc.revistaAstronomy and Astrophysicses_ES
dc.rightsacceso abierto
dc.subjectGalaxies: activees_ES
dc.subjectGalaxies: formationes_ES
dc.subjectGalaxies: evolutiones_ES
dc.subjectGalaxies: star formationes_ES
dc.titleThe dependence of mass and environment on the secular processes of AGNs in terms of morphology, colour, and specific star-formation ratees_ES
dc.typeartículo
dc.volumenVol. 620
sipa.codpersvinculados121221
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