The evolution of the lithium abundances of solar-type stars. IV - Praesepe
Echelle observations are presented of lithium in 63 F and G dwarfs of the Praesepe cluster. For stars earlier than about G0V, Praesepe follows the same trends seen in the Hyades, which has approximately the same age and composition. Stars in Praesepe later than about G5V have more Li than their Hyad...
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Veröffentlicht in: | The Astronomical journal 1993-09, Vol.106 (3), p.1080-1086 |
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Sprache: | eng |
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