Antonio Pipino, Francesca Matteucci
Published 2002-10-24Version 1
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.
Comments: 4 pages, 2 figures, to appear in the ''Proceedings of The evolution of galaxies III. From simple approaches to self-consistent models'', Kiel (Germany), 2002
Journal: Astrophys.Space Sci. 284 (2003) 799-802
The Case Against Bimodal Star Formation in Elliptical Galaxies
The Iron Discrepancy in Elliptical Galaxies after ASCA
A Model for the Chemical Evolution of the Galaxy with Refuses
