Observational constraints on the origin of the elements: VIII. Constraining the barium, strontium, and yttrium chemical evolution in metal-poor stars
[Context] The chemical evolution history of slow neutron-capture elements in the Milky Way is still a matter of debate, especially in the metal-poor regime ([Fe/H] < −1).
| Autores: | , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2024 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/357990 |
| Acceso en línea: | http://hdl.handle.net/10261/357990 |
| Access Level: | acceso abierto |
| Palabra clave: | Stars: abundances ISM: abundances Galaxy: abundances Galaxy: evolution Galaxy: stellar |
| Sumario: | [Context] The chemical evolution history of slow neutron-capture elements in the Milky Way is still a matter of debate, especially in the metal-poor regime ([Fe/H] < −1). |
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