The enigma of Li-rich giants and its relation with temporal variations observed in radial velocity and stellar activity signals

Open Access

Fig. C.1

Example of strong correlations found for stars NGC2423No3 (left) and NGC2345No50 (right). NGC2423No3 shows a strong positive correlation between RV and BIS, while NGC23545No50 shows a strong negative correlation between RV and FWHM.

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