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dc.contributor.authorSchmitt, Henrique Robertopt_BR
dc.contributor.authorKinney, Anne Louisept_BR
dc.date.accessioned2015-01-07T02:10:36Zpt_BR
dc.date.issued1996pt_BR
dc.identifier.issn0004-637Xpt_BR
dc.identifier.urihttp://hdl.handle.net/10183/108766pt_BR
dc.description.abstractWe present high-resolution narrow-band [O III] images of Seyfert 1 and Seyfert galaxies, obtained in the Hubble Space Telescope Data Archive. The continuum-subtr cted [O III] images were useto measure the narrow-line region (NLR) sizes and compare them wlth the predtctlons from te Umfied Scheme. This paper shows that the Seyfert 1 NLR sizes are much smaller than the NLR stzes of the Seyfert 2's if they were observed pole-on. We propose that the Unified Scheme inot wrong but rather that the Seyfert 1's may have their torus axes aligned close to the galaxy plane axts.en
dc.format.mimetypeapplication/pdf
dc.language.isoengpt_BR
dc.relation.ispartofThe astrophysical journal. Chicago. Vol. 463, no. 2, pt. 1 (June 1996), p. 498-508pt_BR
dc.rightsOpen Accessen
dc.subjectMateria interestelarpt_BR
dc.subjectGalaxies: activeen
dc.subjectGalaxies: seyferten
dc.subjectGalaxias seyfertpt_BR
dc.subjectGalaxies: structureen
dc.subjectNucleo galaticopt_BR
dc.subjectEspectros astronômicospt_BR
dc.titleA Comparison between the narrow-line regions of Seyfert 1 and Seyfert 2 galaxiespt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb000148735pt_BR
dc.type.originEstrangeiropt_BR


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