The Orientation of Accretion Disks Relative to Dust Disks in Radio Galaxies

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dc.creatorSchmitt, Henrique R.
dc.date2002-11-03
dc.date.accessioned2026-07-07T02:05:59Z
dc.date.available2026-07-07T02:05:59Z
dc.descriptionWe study the orientation of accretion disks, traced by the position angle of the jet, relative to the dust disk major axis in a sample of 20 nearby Radio Galaxies. We find that the observed distribution of angles between the jet and dust disk major axis is consistent with jets homogeneously distributed over a polar cap of 77 degrees.
dc.description2 pages, 1 figure. To appear in "Active Galactic Nuclei, from Central Engine to Host Galaxy", eds Collin, Combes & Shlosman. PASP Conf. Ser
dc.identifierhttps://arxiv.org/abs/astro-ph/0211039
dc.identifierhttp://arxiv.org/abs/astro-ph/0211039
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5275
dc.subjectAstrophysics
dc.titleThe Orientation of Accretion Disks Relative to Dust Disks in Radio Galaxies
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