Chemical evolution of Elliptical Galaxies and the ICM
arXiv:astro-ph/0210542 · doi:10.1023/A:1024037727520
Abstract
We present a new model for the chemical evolution of elliptical galaxies taking into account SN feedback, detailed nucleosynthesis and galactic winds. We discuss the effect of galactic winds on the chemical enrichment of the ICM and compute the energy per particle injected by the galaxies into the ICM.
arXiv comment4 pages, 2 figures, to appear in the ''Proceedings of The evolution of galaxies III. From simple approaches to self-consistent models'', Kiel (Germany), 2002
References in corpus (8)
- New Observations of the Interstellar Medium in the Lyman Break Galaxy MS 1512-cB58
- Nucleosynthesis in Type Ia Supernovae
- Deconvolution of ASCA X-ray data: II. Radial temperature and metallicity profiles for 106 galaxy clusters
- Dynamical and chemical evolution of gas-rich dwarf galaxies
- SNe heating and the chemical evolution of the intra-cluster medium
- Abundance gradients and the role of SNe in M87
- Roles of SNIa and SNII in ICM Enrichment
- Gas, Iron and Gravitational Mass in Galaxy Clusters: The General Lack of Cluster Evolution at z < 1.0