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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Detalles Bibliográficos
Autores principales:	Cora, Sofía Alejandra, Tornatore, Luca, Borgani, Stefano
Formato:	Objeto de conferencia
Lenguaje:	Inglés
Publicado:	2005
Materias:	Ciencias Astronómicas Hybrid Model Galaxy Cluster Metal Enrichment Cluster Temperature Galaxy Formation
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/142767
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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