Published in
Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S267(5), p. 125-125, 2009
DOI: 10.1017/s1743921310005867
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Dusty Structure Around Type 1 AGNs
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Abstract
AbstractWe 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.
