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Evolution of the compact radio source 3C 345

Published online by Cambridge University Press:  19 July 2016

J. Biretta ,
M. Cohen  and
R. Moore
J. Biretta
Affiliation:
California Institute of Technology Pasadena, California 91125
M. Cohen
Affiliation:
California Institute of Technology Pasadena, California 91125
R. Moore
Affiliation:
California Institute of Technology Pasadena, California 91125

Extract

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The quasar 3C 345 is recognized as a strong, variable, superluminal radio source, an optically violent variable, and a weak X-ray source. We present results of VLBI monitoring between 1979 and 1984 at 2.3, 5.0, 10.7, and 22.2 GHz using antennas of the U.S. and European VLBI Networks. These results are interpreted in terms of a relativistic jet model (Biretta 1985; Biretta et al. 1986).

Type
II. Continuum Emission
Information
Symposium - International Astronomical Union , Volume 119: Quasars , 1986 , pp. 157 - 158
Copyright
Copyright © Reidel 1986 

References

Biretta, J. A.: 1985, , California Institute of Technology.Google Scholar
Biretta, J. A. et al: 1983, Nature 306, 42.Google Scholar
Biretta, J. A., Moore, R. L., and Cohen, M. H.: 1986, Astrophys. J., submitted.Google Scholar
Moore, R. L., Readhead, A. C. S., and Bååth, L. B.: 1983, Nature 306, 44.Google Scholar