Fig. 9.
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Distribution of abundance ratios with distance from mid-plate in three age bins. Besides our clusters, we show data from the APOGEE DR16 (Donor et al. 2020), GES (Casali et al. 2019), OCCASO (Casamiquela et al. 2019), and GALAH (Spina et al. 2021) plus SPA results already published (Frasca et al. 2019; Casali et al. 2020; D’Orazi et al. 2020).
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