Hostname: page-component-669899f699-tzmfd Total loading time: 0 Render date: 2025-04-26T21:35:24.947Z Has data issue: false hasContentIssue false
  • English
  • Français

Multi-Component Models for the Structure and Evolution of Spherical Stellar Systems

Published online by Cambridge University Press:  04 August 2017

Emmanuel Davoust
Emmanuel Davoust*
Affiliation:
Observatoire de Besançon, 25044 BESANCON CEDEX, France

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.

We present stationary analytical models for the structure of spherical stellar systems with several mass components. Evolution is simulated by increasing the central velocity of escape. We compare our models to the results of numerical simulations. An observable kinematical effect of mass segregation is pointed out.

Type
May 30: Model System in the Point-Mass Approximation
Information
Symposium - International Astronomical Union , Volume 113: Dynamic of Stars Clusters , 1985 , pp. 317 - 319
Copyright
Copyright © Reidel 1985 

References

Bailey, M.E., MacDonald, J.: 1981. Mon. Not. R. astron. Soc. 194, 195.CrossRefGoogle Scholar
Davoust, E.: 1977. Astron. Astrophys. 61, 391.Google Scholar
Hénon, M.: 1975. IAU Symp. 69, 133.Google Scholar
Kent, S.M., Gunn, J.E.: 1982. Astron. J. 87, 945.CrossRefGoogle Scholar
Kent, S.M., Sargent, W.L.W.: 1983. Astron. J. 88, 697.CrossRefGoogle Scholar
Kondrat'ev, B.P., Ozernoy, L.M.: 1982. Astrophys. Sp. Sci. 84, 431.CrossRefGoogle Scholar
Spitzer, L., Shull, J.M.: 1975. Astrophys. J. 201, 773.CrossRefGoogle Scholar