Emitting gas regions in Mrk 493: An extensive Fe II line emission region

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dc.creatorPopovic, L. C.
dc.creatorSmirnova, A.
dc.creatorIlic, D.
dc.creatorMoiseev, A.
dc.creatorKovacevic, J.
dc.creatorAfanasiev, V.
dc.date2007-01-24
dc.date.accessioned2026-07-07T07:42:43Z
dc.date.available2026-07-07T07:42:43Z
dc.descriptionWe performed 3D spectroscopic observations of Mrk 493 in order to investigate the Fe II emitting region and their possible connection with the Hydrogen emitting region. We found that there is a strong Fe II emission in an extensive region ~ 4" x 4" around Sy 1 nucleus. The Fe II line width indicates that these lines are originated in an intermediate line region.
dc.descriptionTo appear in the Proceedings of "The Central Engine of Active Galactic Nuclei", editors L. C. Ho and J.-M. Wang
dc.identifierhttps://arxiv.org/abs/astro-ph/0701684
dc.identifierhttp://arxiv.org/abs/astro-ph/0701684
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/122548
dc.subjectAstrophysics
dc.titleEmitting gas regions in Mrk 493: An extensive Fe II line emission region
dc.typetext

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