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B2 quasars and relativistic motion

Published online by Cambridge University Press:  19 July 2016

H.R. de Ruiter ,
A. Rogora  and
L. Padrielli
H.R. de Ruiter
Affiliation:
Istituto di Radio Astronomia, Bologna, Italy
A. Rogora
Affiliation:
Dipartimento di Astronomia, University of Bologna, Italy
L. Padrielli
Affiliation:
Istituto di Radio Astronomia, Bologna, Italy

Extract

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Relativistic motion has been established with a certain degree of confidence only on VLBI scales, but its application to larger scales has encountered severe difficulties (see e.g. De Young, 1984).

Type
II. Continuum Emission
Information
Symposium - International Astronomical Union , Volume 119: Quasars , 1986 , pp. 197 - 201
Copyright
Copyright © Reidel 1986 

References

De Young, D.S.: 1984, in Proceedings of NRAO Workshop No.9, Eds. Bridle, A.H. and Eilek, J.A., p.100 Google Scholar
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Rogora, A., Padrielli, L., de Ruiter, H.R.: 1985a, submitted to Astron. Astrophys. Suppl. Google Scholar
Rogora, A., Padrielli, L., de Ruiter, H.R.: 1985b, in preparation Google Scholar
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