Metal Abundances in the cool-cores of Galaxy Clusters

Details Metal Abundances in the cool-cores of Galaxy Clusters Metal Abundances in the cool-cores of Galaxy Clusters

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1248..287d&link_type=abstract

X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Confer

Astronomy and Astrophysics

Astronomy

Clusters Of Galaxies, Supernovae, Brightness, Interstellar Matter, Galaxy Clusters, Supernovae, Luminosities, Magnitudes, Effective Temperatures, Colors, And Spectral Classification, Intracluster Matter, Cooling Flows

Scientific paper

We carried out a detailed study of the Si, Fe and Ni abundances in the cool cores of a representative sample of 26 local galaxy clusters using XMM-Newton data. We have evaluated the systematic errors that are related to the instruments, the plasma codes and the spectral modeling and computed the relative contribution of type Ia and core-collapsed supernovae to the enrichment process.

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