Baryons and dark matter halo distributions in ACDM cosmology
We analyse the dark matter (DM) distribution in a ≈ 10 M ⊙alo extracted from a simulation consistent with the concordance cosmology, where the physics regulating the transformation of gas into stars was allowed to change producing galaxies with different morphologies. Although the DM profiles get mo...
Guardado en:
| Publicado: |
2009
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v5_nS262_p404_Pedrosa http://hdl.handle.net/20.500.12110/paper_17439213_v5_nS262_p404_Pedrosa |
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