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Chemodynamical Evolution of the Milky Way

Published online by Cambridge University Press:  26 May 2016

Chiaki Kobayashi ,
Naohito Nakasato  and
Ken'ichi Nomoto
Chiaki Kobayashi
Affiliation:
Department of Astronomy, School of Science, University of Tokyo
Naohito Nakasato
Affiliation:
Department of Astronomy, School of Science, University of Tokyo Astronomisches Rechen-Institut
Ken'ichi Nomoto
Affiliation:
Department of Astronomy, School of Science, University of Tokyo

Abstract

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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.

Type
Posters
Information
Symposium - International Astronomical Union , Volume 208: Astrophysical Supercomputing using Particle Simulations , 2003 , pp. 419 - 420
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Katz, N., Weinberg, D.H., & Hernquist, L., 1996, ApJS, 105, 19 CrossRefGoogle Scholar
Kobayashi, C., et al. 1998, ApJ, 503, L155 CrossRefGoogle Scholar
Kobayashi, C., Tsujimoto, T., & Nomoto, K. 2000, ApJ, 539, 26 CrossRefGoogle Scholar