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...
Kaydedildi:
| Yayımlandı: | Revista Mexicana de Astronomía y Astrofísica |
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| Asıl Yazarlar: | , , , |
| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
Universidad Nacional Autónoma de México
2001
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| Konular: | |
| Online Erişim: | https://www.redalyc.org/articulo.oa?id=57101137 |
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