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Fig. 6
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Derived age-velocity dispersions for three different 2-kpc-wide annuli (the Sun is located at Rsol = 8.249 kpc) for LMR stars, i.e. stars that are more metal-rich than the ISM’s metallicity at their guiding radius, with Δ[M/H]ISM > 0.1. The colours and the dashed lines are same as in Fig. 4.
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