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The Origin of AGN-IR Emission

Published online by Cambridge University Press:  19 July 2016

L. G. Stenholm
L. G. Stenholm*
Affiliation:
Astronomical Observatory Uppsala University Box 515 S 751 20 Uppsala Sweden Swedish Defence Research Establishment S 172 90 Sundbyberg Sweden

Abstract

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Advanced multi dimension radiative transfer calculations for an AGN source with a dust disk shows that the AGN-IR emission can be due to reradiation from heated dust in a thick disk. The models produces a weak silicate feature for a wide range of physical conditions, in agreement with the observations.

Keywords

Radiative TransferDustIRAGN
Type
Poster Contributions: Continuum studies
Information
Symposium - International Astronomical Union , Volume 159: Multi-Wavelength Continuum Emission of AGN , 1994 , pp. 336
Copyright
Copyright © Kluwer 1994