Preservation of cuspy profiles in disk galaxy mergers
We carried out three self-consistent N-body simulations of galaxy mergers,with a cuspy dark matter profile, in order to study if the inner dark density slopeis preserved in the remnants. In these simulations the progenitors include botha stellar disk and an intrinsic angular momentum for the halos,...
Guardat en:
| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autors principals: | , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2006
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57142105 |
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