Abstract
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.
| Original language | English |
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| Title of host publication | Astrophysical Supercomputing Using Particle Simulations |
| Editors | J. Makino, P. Hut |
| Place of Publication | SAN FRANCISCO |
| Publisher | Astronomical Society of the Pacific |
| Pages | 419-420 |
| Number of pages | 2 |
| ISBN (Print) | 1-58381-139-7 |
| Publication status | Published - 2003 |
| Event | 208th Symposium of the International Astronomical Union - Tokyo, Japan Duration: 10 Jul 2001 → 13 Jul 2001 |
Conference
| Conference | 208th Symposium of the International Astronomical Union |
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| Country/Territory | Japan |
| City | Tokyo |
| Period | 10/07/01 → 13/07/01 |