On the Infrared Properties of Dusty Torus

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dc.creatorVidela, L.
dc.creatorLira, P.
dc.creatorAlonso-Herrero, A.
dc.creatorAlexander, D. M.
dc.creatorWard, M.
dc.date2006-12-21
dc.date.accessioned2026-07-07T07:36:28Z
dc.date.available2026-07-07T07:36:28Z
dc.descriptionWe performed imaging on 49 type 2 Seyfert galaxies in 6 near- and mid-infrared bands (1-10$μ$m). We are separating the contribution of the torus from the host galaxy by radial profile fitting techniques and we will compare the observed spectral energy distributions with theoretical models of torus emission to constrain geometrical and physical parameters.
dc.descriptionConference proceedings to appear in "The Central Engine of Active Galactic Nuclei", ed. L. C. Ho and J.-M. Wang (San Francisco: ASP)
dc.identifierhttps://arxiv.org/abs/astro-ph/0612646
dc.identifierhttp://arxiv.org/abs/astro-ph/0612646
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/120437
dc.subjectAstrophysics
dc.titleOn the Infrared Properties of Dusty Torus
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