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The Optical and Infrared Properties of 3CR Radio Galaxies
Published online by Cambridge University Press: 14 August 2015
Extract
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).
- 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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