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The Optical and Infrared Properties of 3CR Radio Galaxies

Published online by Cambridge University Press:  14 August 2015

S. J. Lilly  and
M. S. Longair
S. J. Lilly
Affiliation:
Department of Astronomy, University of Edinburgh Blackford Hill, Edinburgh, Scotland
M. S. Longair
Affiliation:
Department of Astronomy, University of Edinburgh Blackford Hill, Edinburgh, Scotland

Extract

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For the last 20 years, a huge observational effort has been devoted to the identification of all 3CR radio sources lying in directions away from the Galactic plane. The project is now more-or-less complete thanks to high-resolution radio observations with aperture synthesis radio telescopes, in particular the Cambridge 5-km telescope, and the use of a CCD camera on the Palomar 5-metre telescope (see e.g. Gunn et al 1980).

Information

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 97: Extragalactic Radio Sources , 1982 , pp. 413 - 422
Copyright
Copyright © Reidel 1982 

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