Chemical evolution with radial mixing
Models of the chemical evolution of our Galaxy are extended to include radial migration of stars and flow of gas through the disc. The models track the production of both iron and α-elements. A model is chosen that provides an excellent fit to the metallicity distribution of stars in the Geneva-Cope...
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| Format: | Journal article |
| Language: | English |
| Published: |
Wiley-Blackwell
2009
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