The classical Hyades lithium problem resolved?

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Abundance, Lithium, Pre-Main Sequence Stars, Stellar Evolution, Stellar Interiors, Stellar Models, Dwarf Stars, G Stars, Mass To Light Ratios, Predictions

Scientific paper

Recent observations of Hyades stars indicate an enhanced oxygen-to-iron ratio in comparison to the Sun. We show that the impact of such an oxygen enhancement on the predictions of pre-main-sequence lithium burning, via interior opacities, is quite substantial. For the first time, self-consistent predictions of the G and K dwarf (Li, Teff) relationship for the Hyades match the observations. Other elements which could be of importance in this regard, for any cluster, are also identified.

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