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Fig. 12.

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Comparison between the measured chemical abundance pattern, [X/Fe], of the star AS0039 (red) in LTE (squares) and NLTE (stars) with model predictions (lines) for the pure descendants of a Pop III 20 M star with fixed mixing fmix = 0.063. Different colours denote different SN explosion energies for Pop III stars: 0.3 × 1051 erg (blue), 1.2 × 1051 erg (green), 5 × 1051 erg (yellow), and 10 × 1051 erg (orange).

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