University of Hertfordshire

By the same authors

Models of Dusty Discs in Active Galactic Nuclei

Research output: Chapter in Book/Report/Conference proceedingConference contribution

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Original languageEnglish
Title of host publicationIn: Procs of the First Stromlo Symposium: The Physics of Active Galaxies.
PublisherAstronomical Society of the Pacific
Pages261-2
ISBN (Print)0-937707-73-2
Publication statusPublished - 1994

Abstract

One of the challenges faced by unified theories for Active Galactic Nuclei (AGN) is to match the observed infrared emission to that predicted for the optically and geometrically thick dusty discs believed to obscure the central source of radiation. We have used the method of Efstathiou & Rowan-Robinson (1990), generalised to take into account a distribution of grain species and sizes (Efstathiou & Rowan-Robinson 1993), to compute models that assume different density distributions. The method treats multiple scattering from grains.

Notes

Original paper can be found at: http://www.astrosociety.org/pubs/cs/035-069.html--Copyright Astronomical Society of the Pacific

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