Low luminosity AGN as seen by IUE

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dc.contributor.authorRodríguez-Pascual, P. M.
dc.date.accessioned2017-03-11T15:39:49Z
dc.date.available2017-03-11T15:39:49Z
dc.date.issued1998
dc.description.abstractDuring its lifetime, IUE has not solved the puzzle of the low luminosity active galactic nuclei. Rather, it has contributed to increase the number of unanswered questions and to reject some ideas obtained from observations in other wavelength ranges. Among LINERs IUE has found very different observational properties, pointing to the presence/co-existence of several gas ionization/powering mechanisms. A relation between AGN-like and star formation activity is strongly suggested by the measured UV fluxes in Seyfert 2 galaxies. Finally, IUE data demonstrates the presence of high velocity gas in the nucleus of Narrow Line Seyfert 1 galaxies, that was questioned by optical observations.spa
dc.description.filiationUEMspa
dc.description.impact0.182 JCR (1998) Q3, 16/28 Aerospace Engineering & Technologyspa
dc.description.sponsorshipSin financiaciónspa
dc.identifier.citationRodríguez-Pascual, P. (1998). Low Luminosity AGN as Seen by IUE. European Space Agency, 413, 595spa
dc.identifier.issn03764265
dc.identifier.urihttp://hdl.handle.net/11268/6245
dc.language.isoengspa
dc.peerreviewedSispa
dc.relation.publisherversionhttp://articles.adsabs.harvard.edu/pdf/1998ESASP.413..595Rspa
dc.rights.accessRightsopen accessen
dc.subject.uemGalaxiasspa
dc.subject.uemAstronomíaspa
dc.subject.uemAstrofísicaspa
dc.subject.unescoGalaxiaspa
dc.subject.unescoAstronomíaspa
dc.subject.unescoAstrofísicaspa
dc.titleLow luminosity AGN as seen by IUEspa
dc.typejournal articlespa
dspace.entity.typePublication

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