A Comparison between the narrow-line regions of Seyfert 1 and Seyfert 2 galaxies
dc.contributor.author | Schmitt, Henrique Roberto | pt_BR |
dc.contributor.author | Kinney, Anne Louise | pt_BR |
dc.date.accessioned | 2015-01-07T02:10:36Z | pt_BR |
dc.date.issued | 1996 | pt_BR |
dc.identifier.issn | 0004-637X | pt_BR |
dc.identifier.uri | http://hdl.handle.net/10183/108766 | pt_BR |
dc.description.abstract | We 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.mimetype | application/pdf | |
dc.language.iso | eng | pt_BR |
dc.relation.ispartof | The astrophysical journal. Chicago. Vol. 463, no. 2, pt. 1 (June 1996), p. 498-508 | pt_BR |
dc.rights | Open Access | en |
dc.subject | Materia interestelar | pt_BR |
dc.subject | Galaxies: active | en |
dc.subject | Galaxies: seyfert | en |
dc.subject | Galaxias seyfert | pt_BR |
dc.subject | Galaxies: structure | en |
dc.subject | Nucleo galatico | pt_BR |
dc.subject | Espectros astronômicos | pt_BR |
dc.title | A Comparison between the narrow-line regions of Seyfert 1 and Seyfert 2 galaxies | pt_BR |
dc.type | Artigo de periódico | pt_BR |
dc.identifier.nrb | 000148735 | pt_BR |
dc.type.origin | Estrangeiro | pt_BR |
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