Simulaciones de fusiones de galaxias en cúmulos
We consider galaxy merging in a cluster under the condition of Aarseth & Fall (1980). The models include the presence of dark matter, which is simulated by a Schuster's radial density law. We present the results obtained from full N-body numerical simulations.
Guardado en:
| Autores principales: | , , |
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1987
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/132196 |
| Aporte de: |
| Sumario: | We consider galaxy merging in a cluster under the condition of Aarseth & Fall (1980). The models include the presence of dark matter, which is simulated by a Schuster's radial density law. We present the results obtained from full N-body numerical simulations. |
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