Contribution of Type Ia and Type II Supernovae for Intra-Cluster Medium Enrichment

Abstract

The origin of the chemical composition of the intracluster medium (ICM) is discussed in this paper. In particular, the contribution from Type Ia supernovae (SNe Ia) to the ICM enrichment is shown to exist by adopting the fitting formulas which have been used in the analysis of the solar system abundances. Our analysis means that we can use the frequency of… (More)

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Cite this paper

@inproceedings{Nagataki1998ContributionOT, title={Contribution of Type Ia and Type II Supernovae for Intra-Cluster Medium Enrichment}, author={Shigehiro Nagataki and Katsuhiko Sato}, year={1998} }