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Polarization Properties of Active Galactic Nuclei

Published online by Cambridge University Press:  12 April 2016

J. H. Hough
J. H. Hough*
Affiliation:
Department of Physical Sciences, University of Hertfordshire, Hatfield, AL1O 9AB, UK

Abstract

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One of the main uses of polarimetry over the last decade, has been to identify the nature of AGN that are normally hidden from direct view by an optically and geometrically thick torus, and thereby to unify different classes of AGN. Of growing importance is the role that polarimetry can play in our understanding of the properties and structure of AGN on a size scale which cannot be resolved directly. We review the progress being made in understanding the role of disks, extended scattering regions, and the obscuring torus in AGN.

Type
Part 13. Large and Small Scale Disks in AGN
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 600 - 609
Copyright
Copyright © Astronomical Society of the Pacific 1997

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