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dc.contributor.authorMaksym, W. Peterpt_BR
dc.contributor.authorFabbiano, Giuseppinapt_BR
dc.contributor.authorElvis, Martinpt_BR
dc.contributor.authorKarovska, Margaritapt_BR
dc.contributor.authorPaggi, Alessandropt_BR
dc.contributor.authorRaymond, John Charlespt_BR
dc.contributor.authorWang, Junfengpt_BR
dc.contributor.authorStorchi-Bergmann, Thaisapt_BR
dc.date.accessioned2017-07-05T02:40:58Zpt_BR
dc.date.issued2016pt_BR
dc.identifier.issn0004-637Xpt_BR
dc.identifier.urihttp://hdl.handle.net/10183/163691pt_BR
dc.description.abstractWe mapped the extended narrowline region (ENLR) of NGC 3393 on scales of r  4 (~1 kpc) from the nucleus using emission line images of Hα λ6563, [O III]l5007, and [S II]ll6717, 6731, taken with the Hubble Space Telescope as part of the CHandra survey of Extended Emission line Regions in nearby Seyfert galaxies (CHEERS). By mapping these lines onto a spatially resolved Baldwin–Phillips–Terlevich diagram, we investigate the impact of feedback from a Compton-thick active galactic nucleus on its circumnuclear ISM. We find that the expected Seyfert-like emission within the ionization bicone (3; 770 pc). We also find a new, figure-8-shaped low ionization emission line region (LINER) cocoon enveloping the bicone and defining a sharp (100 pc) transition between higher and lower-ionization zones. These data illustrate the morphological dependence of ionization states of the ENLR relative to bicone and host gas geometries.en
dc.format.mimetypeapplication/pdfpt_BR
dc.language.isoengpt_BR
dc.relation.ispartofThe astrophysical journal. Bristol. Vol. 829, no. 1 (Sept. 2016), 46, 5 p.pt_BR
dc.rightsOpen Accessen
dc.subjectGalaxies: activeen
dc.subjectGalaxias seyfertpt_BR
dc.subjectGaláxia NGC 3393pt_BR
dc.subjectGalaxies: individual (NGC 3393)en
dc.subjectMapeamentos astronômicospt_BR
dc.subjectGalaxies: Seyferten
dc.titleMapping Seyfert and LINER excitation modes in the inner kpc of NGC 3393pt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb001020851pt_BR
dc.type.originEstrangeiropt_BR


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