A non-extensive approach to the stellar rotational evolution – I: F- and G-type stars
The pioneering study by Skumanich showed that the rotational velocity of G-type mainsequence (MS) stars decreases with stellar age according to v sin i ∝ t −1/2. This relationship is consistent with simple theories of angular momentum loss from rotating stars, where an ionized wind is coupled to the...
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| Principais autores: | , |
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| Formato: | article |
| Idioma: | English |
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Oxford University Press
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| Endereço do item: | https://repositorio.ufrn.br/jspui/handle/123456789/29106 |
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