Fig. 10
Oxygen abundances (in number) after 500 Myr of evolution for “H” models as a function of initial baryonic mass. Symbols are as in Fig. 9. The abundances in the cold (T < 2 × 104 K) phase are shown in the lower set of points (connected by red lines). The abundances in the hot (T > 2 × 104 K) phase are shown in the upper set of points (connected by blue lines).
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