Fig. 4
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Run of a fraction of electrons provided by H (upper panels) and Mg (lower panels) as a function of log τRoss for the model atmospheres of a dwarf (Teff=6500 K and log g=4.5, left panels) and a giant star(Teff=4500 K and log g=1.5, right panels). The colour-coding is according to the metallicity of [M/H]. We adopted [α/Fe]=+0.0 dex for all the models.
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