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dc.contributor.authorSabater, J.
dc.contributor.authorLeon, S.
dc.contributor.authorVerdes-Montenegro, L.
dc.contributor.authorBergond, G.
dc.contributor.authorCarpio, J.
dc.contributor.authorCombes, F.
dc.contributor.authorEspada, D.
dc.contributor.authorGarcía, E.
dc.contributor.authorHuchtmeier, W.
dc.contributor.authorLisenfeld, Ute
dc.contributor.authorSantander-Vela, J. D.
dc.contributor.authorSulentic, J.
dc.contributor.authorVerley, S.
dc.date.accessioned2013-10-11T13:05:06Z
dc.date.available2013-10-11T13:05:06Z
dc.date.issued2006
dc.identifier.citationSabater, J.; et al. Active galaxies in a complete sample of isolated galaxies [póster]. In: Meeting "Visions for infrared astronomy", Paris (France) march 2006. [http://hdl.handle.net/10481/28426]es_ES
dc.identifier.urihttp://hdl.handle.net/10481/28426
dc.description.abstractGalaxy evolution depends strongly on the environment, in particular, galaxy-galaxy interaction can induce nuclear activity by removing angular momentum from the gas so feeding the central black hole. Hence a higher rate of nuclear activity is expected in interacting galaxies. Different studies of this topic lead to contradictory results. Some works conclude that galaxies hosting an active galactic nuclei (AGN) have a higher rate of companions than non active ones. On the other hand other studies do not find this excess of interacting companion or find it only marginally. Most recente works find a different result depending on the type of Seyfer galaxy.es_ES
dc.language.isoenges_ES
dc.rightsCreative Commons Attribution-NonCommercial-NoDerivs 3.0 Licensees_ES
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es_ES
dc.subjectGalaxies es_ES
dc.subjectActivees_ES
dc.subjectIsolatedes_ES
dc.subjectPósteres_ES
dc.titleActive galaxies in a complete sample of isolated galaxieses_ES
dc.typeinfo:eu-repo/semantics/otheres_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES


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