Fig. 13
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Abundance ratios of C,N, Na, and Mg/O as a function of remnant mass for a zero-metallicity 15 M⊙ (top) and 35 M⊙ (bottom) star (Limongi & Chieffi 2012) after the explosion (bold sold lines, left y-axis). The abundance ratio X/O is defined as the difference between the predicted and observed [X/O] values. The right y-axis shows postexplosion interior profiles of 4He (dotted black line), 12C (red), 16O (cyan), 23Na (blue), and 24Mg (orange).
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