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High Resolution Observations of Sub-Kiloparsec Circumnuclear Gas in AGN

Published online by Cambridge University Press:  13 May 2016

J.E. Conway
J.E. Conway*
Affiliation:
Onsala Space Observatory, Onsala, Sweden

Abstract

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In recent years it has become possible to use high resolution radio interferometry and other techniques to study the sub-kiloparsec scale circumnuclear gas in the centres of Active Galactic Nuclei. This gas presumably provides the fuel source for the AGN activity and also plays a role in obscuring the direct view of the central engine from certain directions. The status of high resolution observations of the ionised, atomic and molecular phases of this circumnuclear gas are briefly reviewed.

Type
The Inner Regions of Galaxies
Information
Symposium - International Astronomical Union , Volume 205: Galaxies and their Constituents at the Highest Angular Resolutions , 2001 , pp. 182 - 189
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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