Chemical Evolution and Abundance Ratios in Different Types of Galaxies

Details Chemical Evolution and Abundance Ratios in Different Types of Galaxies Chemical Evolution and Abundance Ratios in Different Types of Galaxies

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..374...89m&link_type=abstract

From Stars to Galaxies: Building the Pieces to Build Up the Universe. ASP Conference Series, Vol. 374, proceedings of the confer

Mathematics

Logic

5

Scientific paper

We will discuss how we can derive very important constraints on galaxy formation and evolution by studying some crucial abundance ratios in galaxies. In particular, we will describe the results obtained by detailed chemical evolution models of galaxies of different morphological type concerning mainly [α/Fe] ratios and how we can use them to understand galaxy evolution and to infer the nature of high redshift objects.

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