Fig. 7.
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[X/Fe] for abundances derived from neutral lines for a Zn-poor (RVS709, open circles), a Zn-normal (RVS728, cross symbols), and a Zn-rich (RVS740, plus symbols) star. We also show the theoretical yields of Heger & Woosley (2002) for stellar masses of 168 M⊙ (green lozenges and line), 195 M⊙ (blue lozenges and line), and 242 M⊙ (red lozenges and line).
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