Fig. 11.
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Predicted surface stellar mass density ΔM⋆ formed in age intervals of 0.05 Gyr as a function of the [Mg/Fe] abundance ratio predicted by the ES21 model (green solid line) and by the M2 model of ES20 (magenta solid line). Colour-coded points correspond to different ages of the SSPs. Vertical dashed lines depict the associated maximum ΔM⋆ values in the high-α sequence stars.
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