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Fig. 3

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Average azimuthal velocity dispersion as a function of the selected percentage of a bin composed of 100 stars, characterised by ⟨ [Fe/H] ⟩ = −0.54 dex, ⟨ [Mg/Fe] ⟩ = +0.17 dex, and σφ = 28 ± 2 km s-1. The error bars correspond to the standard deviation of 1000 bootstrap realisations.

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