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The Sub-Parsec-Scale Structure and Evolution of Centaurus A at 8.4 and 22.2 GHz
Published online by Cambridge University Press: 12 April 2016
Abstract
We have been observing the sub-parsec-scale radio jet in the nucleus of Centaurus A, the closest active radio galaxy, at 8.4 GHz over the last 6 years with the SHEVE array and most recently with the VLBA at 8.4 and 22.2 GHz. In this paper we will review the results of these observations and give a brief summary of our interpretation, concentrating on the evolution of the sub-parsec-scale jet structure with time; subluminal component motions and rapid short timescale evolution. A full description of this work is soon to be published in a major journal article.
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- Research Article
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- Copyright © Astronomical Society of the Pacific 1998