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| Format: | Artículo científico |
| Language: | en |
| Published: |
Universidad Nacional Autónoma de México
2009
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| Online Access: | https://www.redalyc.org/articulo.oa?id=57115758069 |
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Table of Contents:
- NUMERICAL SIMULATIONS OF GALAXY FORMATION IN A ¿ COLD DARK MATTER UNIVERSE M. G. Abadi Física, Astronomía y Matemáticas methods: n hydrodynamics body simulations Galaxies: formation galaxies: structure The success of the A Cold Dark Matter model in reproducing observational results from the large scale structure of the Universe has established it as the new paradigm for galaxy formation and evolution. Cosmological gravitational/hydrodynamical numerical simulations are an invaluable tool to study the origin and evolution of di erent galactic components in this cosmological framework. In the following we review the main ideas presently accepted regarding galaxy formation, and stress the importance of di erent complex astrophysical e ects usually invoked during this process. We emphasise, as well, the fundamental role that satellite accretion events play in shaping the formation of galactic systems. 2009 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57115758069 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.35