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Fig. 11.

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Same as Fig. 10 except the vertical axis is the initial helium mass fraction Yproto, which corresponds to the primordial helium abundance of the protosolar molecular cloud core. The gray open circles in panel d show the results of models K2, K2′, K2-MZvar, K2-MZ1′, and K2-MZ8′ with A2 = [0.12, 0.18].

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