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Properties of Radio Source Host Galaxies

Published online by Cambridge University Press:  05 March 2013

Wim de Vries
Wim de Vries*
Affiliation:
Lawrence Livermore National Laboratory, IGPP, 7000 East Avenue, Livermore, CA 94550, USA.
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Abstract

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A brief overview of the current radio source host galaxy state of affairs is given. All the evidence appears to point towards a scenario in which the young radio source expands through the host galaxy on timescales of 105–106 yr, before it ends its life as a large scale FR II radio galaxy. The place and role of the quasars in this evolutionary picture is unclear, however, and remains an issue of debate.

Keywords

galaxies: activegalaxies: nucleiradio continuum: galaxies
Type
GPS/CSS Workshop
Information
Publications of the Astronomical Society of Australia , Volume 20 , Issue 1 , 2003 , pp. 6 - 11
Copyright
Copyright © Astronomical Society of Australia 2003

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