The origin of stellar populations in the Galactic bulge from chemical abundances
In this work, we study the formation and chemical evolution of the Galactic bulge with particular focus on the abundance pattern ([Mg/Fe] versus [Fe/H]), metallicity, and age distribution functions. We consider detailed chemical evolution models for the Galactic bulge and inner disc, with the aim of...
| Autores principales: | , , , , , , |
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| Formato: | Artículo (Article) |
| Idioma: | Inglés (English) |
| Publicado: |
2025
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| Materias: | |
| Acceso en línea: | https://repositorio.uc.cl/handle/11534/100928 |