Chemodynamical Evolution of Galaxies

Details Chemodynamical Evolution of Galaxies Chemodynamical Evolution of Galaxies

Feb 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sgyu.conf...51k&link_type=abstract

Studies of Galaxies in the Young Universe with New Generation Telescope, Proceedings of Japan-German Seminar, held in Sendai, Ja

Physics

Scientific paper

We discuss the chemodynamical evolution of the Galaxy using our GRAPE-SPH code. It treats dark matter, gas, star particles and contains the physical processes of cooling, star formation, feedback from Type Ia and II supernovae (SNe Ia and II) and stellar winds, and chemical enrichment. For SNe Ia, we adopt the single degenerate scenario with the metallicity effect. We construct the detailed model of the formation and evolution of the Galaxy and compare a number of observational properties, such as age-metallicity relation, the evolutionary change in the abundance ratio, and the metallicity number distribution.

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