Hostname: page-component-848d4c4894-75dct Total loading time: 0 Render date: 2024-06-06T17:22:28.081Z Has data issue: false hasContentIssue false
  • English
  • Français

Modelling Clusters of Galaxies

Published online by Cambridge University Press:  25 April 2016

P. F. Teague  and
D. Carter
P. F. Teague
Affiliation:
Mount Stromlo and Siding Spring Observatories, Australian National University, Canberra
D. Carter
Affiliation:
Mount Stromlo and Siding Spring Observatories, Australian National University, Canberra
Get access Rights & Permissions [Opens in a new window]

Abstract

Thorough investigation of clusters of galaxies involves the complete modelling of their dynamics and structure. Presented here is a description of such a substantial project utilizing a sample of several rich southern clusters of galaxies. Incorporating results from radial velocity analyses of cluster galaxies and X-ray images of the clusters into rigorously constructed models of the cluster potential well and atmosphere will enable the dynamics, structure and evolution of clusters to be tied down.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 6 , Issue 2 , 1985 , pp. 198 - 202
Copyright
Copyright © Astronomical Society of Australia 1985

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

Bancali, N. A., 1975, Astrophys. J., 198, 249.Google Scholar
Bancali, J. N., and Sarazin, C. J., 1977, Astrophys. J. Lett., 213, L99.Google Scholar
Carter, D., and Teague, P. F., 1984, Proc. Astron. Soc. Aust., 5, 502.Google Scholar
Cavaliere, A., and Fusco-Femiano, R., 1976, Astron. Astrophys., 49, 137.Google Scholar
Cavaliere, A., and Fusco-Femiano, R., 1981, Astron. Astrophys., 100, 194.Google Scholar
Cowie, L. L., and Binney, J. J., 1977, Astrophys. J., 215, 723.Google Scholar
Danese, L., De Zotti, G., and di Tullio, G., 1980, Astron. Astrophys., 82, 322.Google Scholar
Fabian, A. C., and Nulsen, P. E. J., 1977, Mon. Not. R. Astron. Soc, 180, 479.CrossRefGoogle Scholar
Gorenstein, P., Fabricant, D., Topka, K., Harnden, F. R., Tucker, W. H., 1978, Astrophys. J., 224, 718.Google Scholar
Gray, P. M., 1983. Proc. S. P. I. E., 374.Google Scholar
Gull, S. F., and Northover, K. J. E., 1975, Mon. Not. R. Astron. Soc, 173, 585.Google Scholar
Kent, S. M., and Gunn, J. E., 1982, Astron. J., 87, 945.Google Scholar
Kent, S. M., and Sargent, W. L. W., 1983, Astron. J., 88, 697.Google Scholar
King, I. R., 1966, Astron. J., 76, 64.Google Scholar
King, I. R., 1972, Astrophys. J. Lett., 174, L123.Google Scholar
Lea, S. M., Silk, J., Kellogg, E., Murray, S., 1973, Astrophys. J. Lett., 184, L105.Google Scholar
Lea, S. M., 1975, Astrophys, J. Lett., 16, 141.Google Scholar
Malumuth, E. M., and Richstone, D. O., 1984, Astrophys. J., 276, 413.CrossRefGoogle Scholar
Matthews, W. G., and Bregman, J. N., 1978, Astrophys. J., 224, 308.Google Scholar
Merritt, D., 1983, Astrophys. J., 264, 24.Google Scholar
Merritt, D., 1984, Astrophys. J., 276, 26.Google Scholar
Richstone, D. O., and Malumuth, E. M., 1983, Astrophys. J., 268, 30.CrossRefGoogle Scholar
Rood, H. J., Page, T., Kintner, E. C., King, I. R., 1972, Astrophys. J., 175, 637.Google Scholar
Strimpel, O., and Binney, J. J., 1979, Mon. Not. R. Astron. Soc, 188, 883.Google Scholar
Tonry, J., and Davis, M., 1979, Astron. J., 84, 1511.Google Scholar
Yahil, A., and Ostriker, J. P., 1973, Astrophys. J., 185, 787.Google Scholar
Zwicky, F., 1957, Morphological Astronomy, Berlin: Springer-Verlag.CrossRefGoogle Scholar