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dc.contributor.authorStorchi-Bergmann, Thaisapt_BR
dc.contributor.authorBonatto, Charles Josept_BR
dc.date.accessioned2014-03-13T01:50:39Zpt_BR
dc.date.issued1991pt_BR
dc.identifier.issn0035-8711pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/88372pt_BR
dc.description.abstractUsing narrow-band imagery, we have detected a cone of radiation in the [O III]λ5007 tine in the nuclei of NGC 1365 and 7582 with emission directed, respectively, towards the south-east and south-west. Adopting a distance of 20 Mpc to NGC 1365 and 21 Mpc to NGC 7582, with H 0 = 75 km s- 1 Mpc - 1 the projected dimensions of the cones are about 1.0 x 1.5 and 1.9 x 1.6 kpc, respectively. The presence of these cones had been previously suggested on the basis of images obtained with the TAURUS Fabry-Perot interferometer and spectroscopic observations, and can be clearly seen in our images after the subtraction of the continuum emission. These observations are new examples of cone morphologies of high-excitation gas previously found in other Seyfert 2 galaxies. The analysis of the available data on NGC 1365 and 7582 favours the so-called 'unified AGN models'.en
dc.format.mimetypeapplication/pdfpt_BR
dc.language.isoengpt_BR
dc.relation.ispartofMonthly notices of the Royal Astronomical Society. Oxford. Vol. 250, no. 1 (May 1991), p. 138-143pt_BR
dc.rightsOpen Accessen
dc.subjectAstrofísicapt_BR
dc.subjectGalaxias seyfertpt_BR
dc.titleDetection of an [O III] λ5007 radiation cone in the nuclei of NGC 1365 and 7582pt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb000055059pt_BR
dc.type.originEstrangeiropt_BR


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