Rotation and lithium abundance of solar-analog stars: Theoretical analysis of observations
Context. Rotational velocity, lithium abundance, and the mass depth of the outer convective zone are key parameters in the study of the processes at work in the stellar interior, in particular when examining the poorly understood processes operating in the interior of solar–analog stars. Aims. We in...
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| Principais autores: | , , |
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| Formato: | article |
| Idioma: | English |
| Publicado em: |
Astronomy & Astrophysics
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| Endereço do item: | https://repositorio.ufrn.br/jspui/handle/123456789/28998 https://doi.org/10.1051/0004-6361/200811026 |
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