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Superluminal Motion in Weak Quasar Cores

Published online by Cambridge University Press:  04 August 2017

R. W. Porcas
R. W. Porcas*
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, F.R.G.

Abstract

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The importance of studying the statistics of the occurrence of superluminal motion in an unbiased sample of radio sources is stressed, and methods for selecting such samples are reviewed. The weak radio cores of quasars exhibiting extended, double-lobed emission can be used for this purpose. Recent studies of the superluminal motion in the core of 3C 179, a quasar selected from such a sample, are described.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 110: VLBI and Compact Radio Sources , 1984 , pp. 157 - 161
Copyright
Copyright © Reidel 1984 

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