ICM METALLICITY EVOLUTION: EFFECTS OF DYNAMICAL PROCESSES
We present a study on the origin of the metallicity evolution of the intracluster medium (ICM) by applying a semi-analytic model of galaxy formation to N-Body/SPH non-radiative cosmological simulations of clusters of galaxies. The results obtained for a set of clusters with virial masses of - 1:5 -...
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
2009
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57115758077 |
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