Chemodynamical evolution of the Milky Way

Kobayashi, C., Nakasato, N. and Nomoto, K. (2003) Chemodynamical evolution of the Milky Way. Astronomical Society of the Pacific.
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We simulate the chemodynamical evolution of the Milky Way using our GRAPE-SPH code, and reproduce the age-metallicity relation, the [O/Fe]-[Fe/H] relation, and the metallicity distribution.

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