Dusty Structure Around Type 1 AGNs

Details Dusty Structure Around Type 1 AGNs Dusty Structure Around Type 1 AGNs

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..267..125m&link_type=abstract

Co-Evolution of Central Black Holes and Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 267

Astronomy and Astrophysics

Astronomy

Galaxies: Active, Quasars: General

Scientific paper

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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