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Maps of Centaurus A from Molonglo and Culgoora

Published online by Cambridge University Press:  25 April 2016

O.B. Slee ,
K.V. Sheridan ,
G.A. Dulk  and
A.G. Little
O.B. Slee
Affiliation:
Division of Radiophysics, CSIRO, Sydney
K.V. Sheridan
Affiliation:
Division of Radiophysics, CSIRO, Sydney
G.A. Dulk
Affiliation:
Division of Radiophysics, CSIRO, Sydney
A.G. Little
Affiliation:
School of Physics, University of Sydney
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Extract

While Centaurus A (NGC 5128) is not a particularly powerful radio galaxy, its proximity (˜ 5 Mpc) permits us to obtain linear resolution an order of magnitude better than can be obtained for the more powerful, distant radio galaxies. Thus one can hope to make meaningful comparisons between the morphologies seen over the electromagnetic spectrum from γ-rays to metre waves. This should lead to a more complete understanding of the energy production mechanisms and evolutionary histories of these objects.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 5 , Issue 2 , 1983 , pp. 247 - 251
Copyright
Copyright © Astronomical Society of Australia 1983

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