Author(s): | Einsel, C. |
Title: | The evolution of rotating collisional systems - application of a parallelized Fokker-Planck-code |
Source: | In: Ebizusaki, T. (ed.): New horizon of computational science Proc. Symp., Tokyo, 1-3 September 1997; Kluwer Academic Publ., Dodrecht, 219-222 |
ISBN: | 0-7923-7050-3 |
Year: | 2001 |
Abstract: | The evolution of initially rotating collisional stellar systems considered as models of flattened globular clusters is followed by means of solving the orbit-average Fokker-Planck equation in two-dimensional (E,Jz)-space. Due to increasingly expensive simulations when utilizing higher numbers of mass bins in the multi-mass case a parallelized version of the code is applied to the problem. Using rotating King-models as starting configurations a stronger mass loss as compared to the non-rotating case may be noticed. The shortest collapse times measured from the models approach the value of 2-3 half-mass relaxation times for rotating models of a large range of King concentration parameters. |
Preprint issued: | |
Remarks: |
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Letzte Änderung/Updated: 02.07.2004