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Superluminal motion in the quasar 3C 279

Published online by Cambridge University Press:  19 July 2016

S. C. Unwin
S. C. Unwin*
Affiliation:
Owens Valley Radio Observatory, California Institute of Technology 105-24, Pasadena, California 91125, USA

Extract

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We present the results of a program of monitoring structure changes in the radio core of the quasar 3C 279 (z = 0.538) using VLBI. In all, nine hybrid maps have been made from observations at frequencies of 5, 11, and 22 GHz, during the period 1981–1985. The VLBI structure shows many similarities with other ‘superluminal’ radio sources, e.g. 3C 273 (Unwin et al. 1985), such as alignment with a kiloparsec-scale jet, a one-sided spectral distribution, and superluminal motion. The proper motion measured from our observations is v/c ≈ 2, only one quarter of the previously published rate.

Type
II. Continuum Emission
Information
Symposium - International Astronomical Union , Volume 119: Quasars , 1986 , pp. 161 - 162
Copyright
Copyright © Reidel 1986 

References

Cotton, W.D., et al.: 1979, Astrophys. J. Letters 229, pp. L115–117.Google Scholar
de Pater, I., and Perley, R.A.: 1983, Astrophys. J. 273, pp. 64–69.Google Scholar
Unwin, S.C., et al.: 1985, Astrophys. J. 289, pp. 109–119.Google Scholar