Metal enrichment of the intracluster medium: A three-dimensional picture of chemical and dynamical properties
We develop a model for the metal enrichment of the intracluster medium (ICM) that combines a cosmological non-radiative hydrodynamical N-body/SPH (smoothed particle hydrodynamic) simulation of a cluster of galaxies, and a semi-analytic model of galaxy formation. The novel feature of our hybrid model...
Guardado en:
| Autor principal: | Cora, Sofía Alejandra |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2006
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/83332 |
| Aporte de: |
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