Chemical evolution of Elliptical Galaxies and the ICM
classification
🌌 astro-ph
keywords
chemicalgalaxiesellipticalevolutiongalacticwindsaccountcompute
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.