Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-26T20:18:51.854Z Has data issue: false hasContentIssue false
  • English
  • Français

Dynamical Models of Elliptical Galaxies

Published online by Cambridge University Press:  14 August 2015

C. P. Wilson
C. P. Wilson*
Affiliation:
Hale Observatories, Carnegie Institution of Washington, California Institute of Technology, Pasadena, Calif., U.S.A.

Abstract

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.

Self-consistent dynamical models of elliptical galaxies have been constructed using a modification of the Prendergast-Tomer algorithm. They reproduce many of the observed properties of elliptical galaxies.

Type
Part II/Flattened Systems
Information
Symposium - International Astronomical Union , Volume 69: Dynamics of Stellar Systems , 1975 , pp. 207 - 208
Copyright
Copyright © Reidel 1975 

References

Burbidge, E. M., Burbidge, G. R., and Fish, R. A.: 1961, Astrophys. J. 134, 251.Google Scholar
Eddington, A. S.: 1915, Monthly Notices Roy. Astron. Soc. 76, 37.Google Scholar
Lynden-Bell, D.: 1967, Monthly Notices Roy. Astron. Soc. 136, 101.Google Scholar
Miller, R. H. and Prendergast, K. H.: 1962, Astrophys. J. 136, 713.Google Scholar
Morton, D. C. and Chevalier, R. A.: 1972, Astrophys. J. 174, 489.Google Scholar
Ostriker, J. P. and Peebles, P. J. E.: 1973, Astrophys. J. 186, 467.Google Scholar
Peterson, C. J.: 1974, private communication.Google Scholar
Prendergast, K. H. and Tomer, E.: 1970, Astron. J. 75, 674.Google Scholar
Wilson, C. P.: 1973, ‘Dynamical Models of Elliptical Galaxies’, , Berkeley .Google Scholar