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Extended Extragalactic Radio Emission

Published online by Cambridge University Press:  26 May 2016

F.N. Owen ,
M.J. Ledlow ,
J.A. Eilek ,
N.E. Kassim ,
N. Miller ,
K.S. Dwarakanath  and
R.J. Ivison
F.N. Owen
Affiliation:
NRAO, P.O. Box O, Socorro, NM 87801 USA
M.J. Ledlow
Affiliation:
University of New Mexico, Albuquerque NM USA
J.A. Eilek
Affiliation:
New Mexico Tech, Socorro, NM 87801 USA
N.E. Kassim
Affiliation:
NRL, Washington, DC USA
N. Miller
Affiliation:
NRAO, P. O. Box O, Socorro, NM 87801 USA
K.S. Dwarakanath
Affiliation:
Raman Institute, Bangalore, India
R.J. Ivison
Affiliation:
University College London, Gower Street, London WC1E 6BT UK

Abstract

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Extended radio emission and its relation to parent galaxy properties is briefly reviewed. Our current understanding of the relation between absolute radio and optical luminosity, radio morphology and linear size is discussed. The impact of radio jets on dense cluster cores is discussed using M87 as an example. Finally, the relation of AGN's to star-bursting galaxies at high redshift is considered.

Type
Part 4: Extragalactic Radio Sources
Information
Symposium - International Astronomical Union , Volume 199: The Universe at Low Radio Frequencies , 2002 , pp. 171 - 178
Copyright
Copyright © Astronomical Society of the Pacific 2002 

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