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.
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References
Dehnen W., 1995, MNRAS, 274, 919
Merritt D., Sellwood J., 1994, ApJ, 425, 551
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© 1996 Springer Science+Business Media Dordrecht
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Dehnen, W. (1996). Bars in Cusps. In: Bender, R., Davies, R.L. (eds) New Light on Galaxy Evolution. International Astronomical Union / Union Astronomique Internationale, vol 171. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0229-9_69
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DOI: https://doi.org/10.1007/978-94-009-0229-9_69
Publisher Name: Springer, Dordrecht
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