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Paper: |
A New Look at Galactic Chemical Signatures of Enrichment and Infall |
Volume: |
240, Gas and Galaxy Evolution: A Conference in Honor of the 20th Anniversary of the VLA |
Page: |
273 |
Authors: |
Oey, M. S. |
Abstract: |
I present a simple, closed-box, analytic model for inhomogeneous chemical evolution that assumes no mixing, but incorporates a contamination filling factor Q. This model shows better agreement with the Galactic disk stellar metallicities than the homogeneous closed-box model. There is also excellent agreement with the halo metallicities, representing a relatively unevolved system. These results offer a revised interpretation of the observed metallicity distributions and details of gas infall. |
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