Fig. 5.
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Lithium abundance as a function of rotational velocity for the full field GES iDR6 stellar sample selected for this paper (3210 objects). The stars are colour-coded according to their effective temperature. Both 7Li measurements (circles) and upper limits (dots) are shown. Rotational velocities are measured from FLAMES-UVES spectra; typical errors on v sin i are ≤5 km s−1.
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