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Two-Dimensional Fokker-Planck Models
Published online by Cambridge University Press: 25 May 2016
Abstract
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The evolution of spherical single-mass star clusters was followed by numerically solving the orbit-averaged two-dimensional Fokker-Planck equation in energy-angular momentum space. Velocity anisotropy is allowed in the two-dimensional Fokker-Planck model. The development of the anisotropy is discussed in detail.
- Type
- Stellar Dynamics, Models
- Information
- Symposium - International Astronomical Union , Volume 174: Dynamical Evolution of Stars Clusters , 1996 , pp. 91 - 100
- Copyright
- Copyright © Kluwer 1996
References
Cohn, H.
1985, in Dynamics of Star Clusters, IAU Symp No.113, ed Goodman, J., Hut, P. (D. Reidel Publishing Company, Dordrecht) p161
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Hut, P.
1985, in Dynamics of Star Clusters, IAU Symp No.113, ed Goodman, J., Hut, P. (D. Reidel Publishing Company, Dordrecht) p231
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