Sensitivity of the orbital content of a model stellar system to the potential approximation used to describe it
We have classified orbits in a stationary triaxial stellar system created from a cold dissipationless collapse of 100,000 particles. In order to integrate the orbits, two potential approximations with different fitting functions were used in turn. We found that the relative amount of chaotic versus...
Guardado en:
| Autores principales: | Carpintero, Daniel Diego, Wachlin, Felipe Carlos |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2006
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/130461 |
| Aporte de: |
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