Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-28T19:52:38.603Z Has data issue: false hasContentIssue false

Isothermal Clusters of Galaxies

Published online by Cambridge University Press:  25 April 2016

B. M. Lewis*
Affiliation:
Carter Observatory, Wellington

Extract

A departure from an isothermal mass distribution in a rich cluster is expected if the genesis involves a coherent recollapse phase. The character of this departure is calculated and looked for in the data available for the Comma Cluster. No significant deviation from an isothermal mass distribution is found for r < 360’.

Type
Extra-galactic
Copyright
Copyright © Astronomical Society of Australia 1978

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Bradley, J. V., Distribution Free Statistical Tests, p. 266 New Jersey, Prentice-Hall (1968).Google Scholar
Lewis, B. M., Proc. Ast. Soc. Aust., 3, 140 (1977).CrossRefGoogle Scholar
Rood, H. J., Page, T. L., Kintner, E. C., and King, I. R., Astrophys. J., 175, 627 (1972).Google Scholar
Tifft, W. G., and Gregory, S. A., Astrophys. J., 205, 696 (1976).Google Scholar
Zwicky, F., Morphological Astronomy; Berlin: Springer-Verlag (1957).Google Scholar