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Numer of Masses and Metallicities in Grids of Stellar Models

Stellar yields are crucial inputs for galactic chemical evolution models. Here we investigate the impact of the stellar remnant mass distribution and the resolution of a set of stellar yields on the evolution of light elements.
Project summary
Study of the impact of the number of masses and metallicities, in a grid of stellar models, on galactic chemical evolution predictions.
About the simulation codes
We used OMEGA (part of NuPyCE).
Link to the published paper