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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

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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