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Two Stationary Components in the High-Redshift Quasar 1338+381

Published online by Cambridge University Press:  12 April 2016

F. Bouchy  and
J.-F. Lestrade
F. Bouchy
Affiliation:
Observatoire de Paris-Meudon, F92195, Meudon, France
J.-F. Lestrade
Affiliation:
Observatoire de Paris-Meudon, F92195, Meudon, France

Abstract

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VLBI observations of the high-redshift quasar 1338+381 reveal a source with two well defined components that are stationary and possibly, a weaker component that moves in between at a very high superluminal speed.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 57 - 58
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

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Shaffer, D.B. 1984. VLBI and Compact Radio Sources; IAU Symposium 110, eds. Fanti, , Kellerman, & Setti, (Dordrecht: Reidel), 365–374.Google Scholar