Hostname: page-component-8448b6f56d-gtxcr Total loading time: 0 Render date: 2024-04-20T03:02:53.717Z Has data issue: false hasContentIssue false
  • English
  • Français

Search for superluminal motion in the weak cores of extended quasars

Published online by Cambridge University Press:  19 July 2016

J. A. Zensus  and
R. W. Porcas
J. A. Zensus
Affiliation:
California Institute of Technology, Pasadena, U.S.A.
R. W. Porcas
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, F.R.G.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present a status report on a project to study structural changes in a sample of radio cores associated with quasars with extended double lobes. Of six objects observed, so far two (3C 179 and 3C 263) are superluminal and two more (3C 268.4 and 1951+49) are possible superluminal candidates.

Type
II. Continuum Emission
Information
Symposium - International Astronomical Union , Volume 119: Quasars , 1986 , pp. 167 - 168
Copyright
Copyright © Reidel 1986 

References

Blandford, R. D. and Königl, A.: 1979, Astrophys. J. 232, 34 Google Scholar
Orr, M. J. L., Browne, I. W. A.: 1982, Monthly Not. Roy. Astron. Soc. 200, 1067 Google Scholar
Owen, F. N., Porcas, R. W., Neff, S. G.: 1978, Astron. J. 83, 1009 Google Scholar
Porcas, R. W.: 1981, Nature 294, 47 Google Scholar
Scheuer, P. A. G. and Readhead, A. C. S.: 1979, Nature 277, 182 Google Scholar
Zensus, J. A. and Porcas, R. W.: 1984, proc. IAU Symp. 110, 163 Google Scholar
Zensus, J. A., Hough, D. H., Porcas, R. W.: 1986, in preparation Google Scholar