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Fig. 8.
Similar to Fig. 7, but N/Fe and AGB yields (orange) are included during the fit. Again, the favoured IMF power-law index is 2.35 (Salpeter) and Zinit = 0.02. The SNIa fraction is consistent with the previous result. The ratio (
) between the number of low- and intermediate-mass stars and that of massive stars is 180 ± 50.
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