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Homology in the Evolution of Cluster Cores

Published online by Cambridge University Press:  14 August 2015

D. Lynden-Bell*
Affiliation:
Institute of Astronomy, The Observatories, Cambridge, U.K.

Abstract

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It is pointed out that in advanced phases of evolution the cores of clusters ought to evolve homologously and reasons are sought as to why this evolution should be at constant core energy. It is pointed out that continued evolution after infinite core densities have been achieved is an important area for future research.

Type
Part I/Spherical Systems
Copyright
Copyright © Reidel 1975 

References

Aarseth, S. J.: 1974, Astron. Astrophys. 35, 237.Google Scholar
Hénon, M.: 1961, Ann. Astrophys. 24, 369.Google Scholar
Hénon, M.: 1969, Astron. Astrophys. 2, 151.Google Scholar
Hénon, M.: 1971, Astrophys. Space Sci. 13, 284.CrossRefGoogle Scholar
Hénon, M.: 1973, in Martinet, L. and Mayor, M. (eds.), Dynamical Structure and Evolution of Stellar Systems, Swiss Society of Astronomy and Astrophysics Third Advanced Course, Geneva Observatory.Google Scholar
King, I. R.: 1958, Astron. J. 63, 114.Google Scholar
King, I. R.: 1966, Astron. J. 71, 64.Google Scholar
Larson, R. B.: 1970, Monthly Notices Roy. Astron. Soc. 150, 93.Google Scholar
Lynden-Bell, D. and Wood, R.: 1968, Monthly Notices Roy. Astron. Soc. 138, 495.Google Scholar
Miller, R. H. and Parker, E. N.: 1964, Astrophys. J. 140, 50.Google Scholar
Spitzer, L. and Thuan, T. X.: 1972, Astrophys. J. 175, 31.CrossRefGoogle Scholar
Spitzer, L.: 1973, Astrophys. J. 183, 565.CrossRefGoogle Scholar
Woolley, R. v. d. R.: 1954, Monthly Notices Roy. Astron. Soc. 114, 191.Google Scholar