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Radio Observations of Clusters of Galaxies

Published online by Cambridge University Press:  25 April 2016

B. Y. Mills  and
R. R. Shobbrook
B. Y. Mills
Affiliation:
Chatterton Astronomy Department, University of Sydney
R. R. Shobbrook
Affiliation:
Chatterton Astronomy Department, University of Sydney
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Extract

High resolution studies of clusters of galaxies at radio frequencies may contribute substantially to our knowledge of the properties of radio galaxies, their evolution and their luminosity function. A considerable amount of statistical information is already available on the correspondence of radio sources and clusters; the present investigation is aimed rather at a detailed examination of the sources and their identification with actual galaxies or other objects.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 1 , January 1967 , pp. 24
Copyright
Copyright © Astronomical Society of Australia 1967

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References

1 Abell, G. O., Ap. J. Supp., 3, No. 31 (1958).Google Scholar
2 Mills, B. Y, Aust. J. Phys., 13, 550–577 (1960).CrossRefGoogle Scholar
3 Shimmins, A., Clarke, Margaret E., and Ekers, R. D., Ausi. J. Phys., 19, 649–686 (1966).Google Scholar