Infrared Observations of AGN
classification
🌌 astro-ph
keywords
propertiescomparedconstraindatadustemissiongalaxiesgeometrical
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We present results from an imaging and spectroscopic study of the dust properties of Seyfert galaxies in the 1-10um range. The data are compared to state of the art models of torus emission to constrain geometrical and physical properties of the obscuring medium.
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