Chemical evolution of the intracluster gas

Details Chemical evolution of the intracluster gas Chemical evolution of the intracluster gas

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.157..221p&link_type=abstract

(Instituto de Astrofisica de Canarias and Comision Interministerial de Ciencia y Tecnologia, Summer School on Evolutionary Pheno

Astronomy and Astrophysics

Astronomy

5

Chemical Evolution, Cosmic Gases, Galactic Clusters, Metallicity, X Ray Astronomy

Scientific paper

Recent X-ray observations have shown that intracluster medium has nonprimordial composition. Iron lines have been detected. Preliminary results on modeling of the chemical evolution of the intracluster medium in galaxy clusters are presented. The Galactic winds driven by supernovae are considered in detail, taking into account the binding energy of the galactic gas. An attempt is made to explain the metallicity gradient observed in the Perseus cluster from morphological segregation of galaxies in the inner part of the cluster.

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