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Radio-Optical Correlations in Distant Radio Galaxies

Published online by Cambridge University Press:  07 August 2017

Wil van Breugel  and
Patrick J. McCarthy
Wil van Breugel
Affiliation:
Department of Astronomy, University of California, Berkeley, CA 94720 U.S.A.
Patrick J. McCarthy
Affiliation:
Department of Astronomy, University of California, Berkeley, CA 94720 U.S.A.

Abstract

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Optical identifications and redshifts are now available for nearly all 3CR radio galaxies (Spinrad et al. 1985; Djorgovski et al. 1988). Using new radio and optical observations, supplemented with data from the literature, we are conducting a systematic comparison of their radio and optical (emission-line and galaxy) properties, and their dependence on redshift. Here we present new results on the alignments of galaxies and their associated radio sources, and radio source asymmetries.

Type
Part 10: Radio Galaxies, Components and Structure
Information
Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 546 - 547
Copyright
Copyright © Kluwer 1989 

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