A simple model for galaxy formation
Numerical experiments concerning the dynamics of a distribution of interacting gas clouds in a proto-galactic potential well are analyzed. Dissipation of energy by means of inelastic cloud collisions produce, after a few free fall times a strong flattening and a large ratio of rotational vs. total k...
Guardado en:
| Autores principales: | Abadi, Mario Gabriel, García-Lambas, D., Mosconi, M., Navarro, J. |
|---|---|
| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1988
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/142268 |
| Aporte de: |
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