Mass effect on the lithium abundance evolution of open clusters: Hyades, NGC 752, and M67
Lithium abundances in open clusters provide an e ective way of probing mixing processes in the interior of solar-type stars and convection is not the only mixing mechanism at work. To understand which mixing mechanisms are occurring in low-mass stars, we test non-standard models, which were calibrat...
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| Autors principals: | , , , |
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| Format: | article |
| Idioma: | English |
| Publicat: |
EDP Sciences
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| Matèries: | |
| Accés en línia: | https://repositorio.ufrn.br/jspui/handle/123456789/29048 |
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