Fig. 6
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Running mean of [P/Fe] for the stars in our sample (blue line) and the Maas et al. (2022) sample (red line) as a function of [Fe/H]. The standard deviation is represented by the blue and red bands for our sample and the Maas et al. (2022) sample, respectively. With a dashed line, we show the chemical evolution trend in Cescutti et al. (2012).
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