Galactic Halo Formation and the Evolution of Bias
We study the evolution of bias in four cosmological models (LambdaCDM, OCDM, tauCDM, and SCDM). The use of very high-resolution simulations, achieved with the AP3M code, produces dozens of galaxy-size halos inside groups. The groups look like real groups of galaxies. The bias decreases monotonically...
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
2001
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57101137 |
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