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Superluminal Motions and Large Scale Structure in 3C 120

Published online by Cambridge University Press:  03 August 2017

R. C. Walker
Affiliation:
National Radio Astronomy Observatory*, Socorro, N.M., U.S.A.
J. M. Benson
Affiliation:
National Radio Astronomy Observatory*, Charlottesville, VA, U.S.A.
S. C. Unwin
Affiliation:
California Institute of Technology, Pasadena, CA, U.S.A.

Abstract

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The jet in the superluminal source 3C 120 has been observed on all scales from under a parsec to about 100 kpc. The jet brightness decays rather smoothly with core distance, indicating that the basic characteristics of the jet are established on parsec or smaller scales and evolve simply with distance.

Type
Extragalactic
Copyright
Copyright © Reidel 1988 

References

Baldwin, J. A., Carswell, R. F., Wampler, E. J., Smith, H. E., Burbidge, E. M., and Boksenberg, A. 1980, Ap. J., 236, 388.CrossRefGoogle Scholar
Bridle, A. H., and Perley, R. A. 1984, Ann. Rev. Astron. Ap., 22, 319.CrossRefGoogle Scholar
Walker, R. C., Benson, J. M., and Unwin, S. C. 1987, Ap. J., 316, 546.Google Scholar
Walker, R. C., Benson, J. M., and Unwin, S. C. 1987, in Superluminal Radio Sources, ed. Zensus, J. A. and Pearson, T. J. (Cambridge: Cambridge University Press), p. 48.Google Scholar