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dc.date.accessioned 2023-11-08T13:07:38Z
dc.date.available 2023-11-08T13:07:38Z
dc.date.issued 1994
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/159917
dc.description.abstract In this communication we present the main results obtained in the study of AGNs showing extreme IR continuum and Fe II emission lines. Furthermore, we discuss that these objects can be young QSOs at the end phase of a strong starburst with superwind and superbubbles (suggested by Lipari, Terlevich &: Machetto 1993). Also, we discuss the origin of broad absorption lines (BAL) systems, associated to the phase of young QSO. en
dc.language es es
dc.subject Galaxia es
dc.title Galaxias con emisión extrema en el IR y Fe II es
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Lípari, S.L. es
sedici.subject.materias Astronomía es
sedici.description.fulltext true es
mods.originInfo.place Asociación Argentina de Astronomía es
sedici.subtype Comunicacion es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.journalTitle Boletín de la Asociación Argentina de Astronomía es
sedici.relation.journalVolumeAndIssue no. 39 es


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