Low luminosity AGN as seen by IUE

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dc.contributor.author Rodríguez-Pascual, P. M.
dc.date.accessioned 2017-03-11T15:39:49Z
dc.date.available 2017-03-11T15:39:49Z
dc.date.issued 1998
dc.identifier.citation Rodríguez-Pascual, P. (1998). Low Luminosity AGN as Seen by IUE. European Space Agency, 413, 595 spa
dc.identifier.issn 03764265
dc.identifier.uri http://hdl.handle.net/11268/6245
dc.description.abstract During 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.sponsorship SIN FINANCIACIÓN spa
dc.language.iso eng spa
dc.title Low luminosity AGN as seen by IUE spa
dc.type article spa
dc.description.impact 0.182 JCR (1998) Q3, 16/28 Aerospace Engineering & Technology spa
dc.rights.accessRights closedAccess en
dc.subject.uem Galaxias spa
dc.subject.uem Astronomía spa
dc.subject.uem Astrofísica spa
dc.subject.unesco Galaxia spa
dc.subject.unesco Astronomía spa
dc.subject.unesco Astrofísica spa
dc.description.filiation UEM spa
dc.peerreviewed Si spa

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