Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-27T04:44:00.435Z Has data issue: false hasContentIssue false
  • English
  • Français

Superluminal Motion in the Parsec-Scale Jet of 3C 380

Published online by Cambridge University Press:  12 April 2016

A.G. Polatidis  and
P.N. Wilkinson
A.G. Polatidis
Affiliation:
Onsala Space Observatory, Onsala, S-43992 SWEDEN and Joint Institute for VLBI in Europe, Dwingeloo, The Netherlands
P.N. Wilkinson
Affiliation:
N.R.A.L., Jodrell Bank, Macclesfield, Cheshire, U.K.

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.

Multi-epoch VLBI observations of the quasar 3C 380 reveal a bent parsec-scale radio jet with complex substructure and superluminal motion out to ~100 pc from the core.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 77 - 78
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Hardee, P.E., & Norman, M.L. 1989. ApJ, 342, 680–685.Google Scholar
Polatidis, A.G., & Wilkinson, P.N. 1997. MNRAS, accepted.Google Scholar
Wilkinson, P.N., et al. 1990. in Parsec-Scale Radio Jets, eds. Zensus, J.A. & Pearson, T.J. (Cambridge: Cambridge Univ. Press), 152–160.Google Scholar
Wilkinson, P.N., et al. 1991. MNRAS, 248, 86–90.Google Scholar
Zensus, J.A., Cohen, M.H., & Unwin, S.C. 1995. ApJ, 443, 35–53.Google Scholar