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We test the correlation between Li-abundance and rotation period for solar-type stars (spectral-type in G0-K0). The result is not unique. Stars in young open clusters (IC2391, IC2602, IC4665, Per) show a clear correlation: the faster the stellar rotation the smaller the Li-depletion. For the Pleiades cluster this correlation is still present but weak. The use of in- verse Rossby number does not change this result.

Rotation-induced lithium depletion of solar-type stars in open stellar clusters