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Superluminal Expansion in 3C 179

  • R. W. Porcas
Part of the International Astronomical Union / Union Astronomique Internationale book series (IAUS, volume 97)

Abstract

The detection of apparent faster-than-light motion (v=7.6c) in the core of 3C 179 poses some problems for the simple relativistic jet explanation.

Keywords

Flux Density Radio Emission Radio Source VLBI Observation Extragalactic Radio Source 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

References

  1. 1.
    Scheuer, P.A.G. and Readhead, A.C.S.: 1979, Nature 277, pp. 182–5ADSCrossRefGoogle Scholar
  2. 2.
    Owen, F.N., Porcas, R.W. and Neff, S.G.: 1978, Astron. J. 83, pp. 1009–20ADSCrossRefGoogle Scholar

Copyright information

© IAU 1982

Authors and Affiliations

  • R. W. Porcas
    • 1
  1. 1.Max-Planck-Institut für RadioastronomieBonnGermany

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