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The Enrichment of the Intracluster Medium | | Brad K. Gibson
; Francesca Matteucci
; | | Date: |
13 Dec 1996 | | Subject: | astro-ph | | Affiliation: | MSSSO), Francesca Matteucci (SISSA | | Abstract: | The enrichment of the intracluster medium (ICM) of galaxy clusters, within the framework of the supernovae-driven wind model for elliptical galaxies, has been considered under two extreme assumptions regarding the binding energy-mass-radius relations. Unless the binding energy at the time of wind commencement, for a given galactic mass, was a factor of approximately five lower than that predicted by the present-day relation, at most 20% of the ICM gas could have originated within the cluster ellipticals themselves, the remainder being of primordial origin. | | Source: | arXiv, astro-ph/9612131 | | Services: | Forum | Review | PDF | Favorites | |
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