Fig. 15

Stellar mass distribution as a function of [Mg/Fe] predicted by the PM04 chemical evolution model for a typical elliptical galaxy (solid line). The luminosity distribution as a function of [Mg/Fe] is given by the dotted line. The dashed line gives the luminosity distribution when the SSPs formed at [Fe/H] < −1 are not taken into account (see text). The curves have been arbitrarily rescaled to the same value and offset to make differences in the tails more visible.
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