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Bars in Cusps

  • Walter Dehnen
Conference paper
Part of the International Astronomical Union / Union Astronomique Internationale book series (IAUS, volume 171)

Abstract

In order to investigate the stability properties of galaxy models with central density cusps, N-body simulations of oblate models with density \(\rho \propto m^{-1} (m+a)^{-3}\) where m 2 =R 2+[z/q]2 and distribution functions f(E,L z) (computed as in Dehnen, 1995) have been performed with the following results.

References

  1. Dehnen W., 1995, MNRAS, 274, 919ADSGoogle Scholar
  2. Merritt D., Sellwood J., 1994, ApJ, 425, 551ADSCrossRefGoogle Scholar

Copyright information

© Springer Science+Business Media Dordrecht 1996

Authors and Affiliations

  • Walter Dehnen
    • 1
  1. 1.Theoretical PhysicsOxfordUK

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