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Fig. 6
Lithium abundance versus vsini for stars observed at high resolution. Symbols as in Fig. 5. Bottom panels show for each group the log n(Li) dispersion as a function of vsini at the following bins: 0–30, 30–60, 60–90, 90–120 km s-1. The values are shifted in vsini to better visualize the symbols.
This figure is made of several images, please see below:
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