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Dusty Structure Around Type 1 AGNs
Published online by Cambridge University Press: 03 June 2010
Abstract
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We present a detailed investigation of the MIR continuum emission of type 1 QSOs and define the main emission components. Our model requires three components: a clumpy torus, dusty narrow-line region (NLR) clouds and a blackbody-like hot dust.
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- Copyright © International Astronomical Union 2010
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