Using rotation, magnetic activity and lithium to estimate the ages of low mass stars
The rotation rate, level of magnetic activity and surface lithium abundance are age-dependent quantities in stars of about a solar mass and below. The physical reasons for the evolution of these phenomena are qualitatively understood, but accurate quantitative models remain dependent on empirical ca...
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| Veröffentlicht in: | EAS publications series 2014-01, Vol.65, p.289-325 |
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| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext |
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