Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-30T03:44:31.371Z Has data issue: false hasContentIssue false
  • English
  • Français

A Morphological Classification of Clusters of Galaxies from Einstein Images

Published online by Cambridge University Press:  14 August 2015

C. Jones  and
W. Forman
C. Jones
Affiliation:
Harvard-Smithsonian Center for Astrophysics
W. Forman
Affiliation:
Harvard-Smithsonian Center for Astrophysics

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The earliest Uhuru observations showed that cluster X-ray sources were not associated with single individual galaxies but were extended sources (Gursky et al. 1971, Kellogg et al. 1972, and Forman et al. 1972). The detection of iron line emission from X-ray spectroscopic observations (Mitchell et al. 1976 and Serlemitsos et al. 1977) showed both that the dominant X-ray emission process was thermal bremsstrahlung and that the gas had been processed through stellar systems before being injected into the intracluster medium.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 97: Extragalactic Radio Sources , 1982 , pp. 97 - 106
Copyright
Copyright © Reidel 1982 

References

Bahcall, N. 1977, Ann. Rev. of Astr. and Astrophys. 15, 505.Google Scholar
Bechtold, J., Forman, W., Giacconi, R., Jones, C., Schwarz, J., Tucker, W., and Van Speybroeck, L. 1981, Ap. J., in press.Google Scholar
Carter, D. and Metcalf, N. 1980, MNRAS, 191, 325.Google Scholar
Elvis, M., Schreier, E., Tonry, J., Davis, M., and Huchra, J. 1981, Ap. J., 246, 20.Google Scholar
Fabricant, D., Lecar, M., and Gorenstein, P. 1980, Ap. J., 241, 552.Google Scholar
Forman, W., Kellogg, E., Gursky, H., Tananbaum, H., and Giacconi, R. 1972, Ap. J., 178, L309.Google Scholar
Forman, W., Schwarz, J., Jones, C., Liller, W., and Fabian, A.C. 1979, Ap. J., 234, L27.Google Scholar
Forman, W., Bechtold, J., Blair, W., Giacconi, R., Van Speybroeck, L., and Jones, C. 1981, Ap. J., 243, L133.Google Scholar
Gavazzi, G. 1978, Astr. Ap., 69, 355.Google Scholar
Gursky, H., Kellogg, E., Murray, S., Leong, C., Tananbaum, H., and Giacconi, R. 1971, Ap. J., 167, L81.CrossRefGoogle Scholar
Hausman, M. and Ostriker, J. 1978, Ap. J., 224, 320.Google Scholar
Jones, C., Mandel, E., Schwarz, J., Forman, W., Murray, S., and Harnden, F.R. Jr. 1979, Ap. J., 234, L21.Google Scholar
Kellogg, E., Tananbaum, H., Giacconi, R., and Pounds, K. 1972, Ap. J., 174, L65.Google Scholar
Leir, A. and van den Berg, S. 1977, Ap.J. Suppl., 34, 381.CrossRefGoogle Scholar
Mitchell, R.J., Culhane, J.L., Davison, P.J.N., and Ives, J.C. 1976, MNRAS, 176, 29p.Google Scholar
Mushotsky, R. and Smith, B. 1980, Highlights of Astronomy, 5, 735.CrossRefGoogle Scholar
Oemler, G. 1980, private communication.Google Scholar
Serlemitsos, P., Smith, B., Boldt, E., Holt, S., and Swank, J. 1977, Ap. J., 211, L63.CrossRefGoogle Scholar
White, S.D.M. 1976, MNRAS, 177, 717.Google Scholar