Fig. 9.
Observed element-to-iron abundance ratios as a function of the [Fe I/H] abundance. Cases where all models fail to represent the data. Shown are the Romano et al. (2010) R1 model (dark green line) and R15 model (light green line), the Kobayashi & Nakasato (2011) thin disc model (magenta line), and the Prantzos et al. (2018) baseline model (grey line).
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