Comparing Semi-Analytical and Numerical Modelling of the ICM Chemical Enrichment
The dependence of iron abundance on cluster temperature is subject to continuous debate. There are some evidences of decreasing abundances from ~0.7 to ~0.3 times the solar metallicity in the temperature range of ~3 — 10 keV, while a roughly constant value of ~0.3 times solar is claimed. Physical in...
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Autores principales: | Cora, Sofía Alejandra, Tornatore, Luca, Borgani, Stefano |
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Formato: | Objeto de conferencia |
Lenguaje: | Inglés |
Publicado: |
2005
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Materias: | |
Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/142767 |
Aporte de: |
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