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The Structure and Evolution of Massive Rotating Single and Binary Population III Stars

  • Authors: Hanfeng Song, Georges Meynet, Zhi Li, Weiguo Peng, Ruiyu Zhang, and Qiong Zhan

2020 The Astrophysical Journal 892 41.

  • Provider: AAS Journals

Caption: Figure 9.

Mass fraction of H, He, C, N, O, and Ne as a function of the mass coordinate for the nonrotational model S2 and rotational model S8 at different evolutionary points as indicated by the different colors: ZAMS (red solid lines); the end of central hydrogen burning (marked by ECHB; green dashed lines); the end of central helium burning (marked by ECHeB; blue dashed lines); the end of calculation (marked by EOC; purple dashed–dotted lines.)

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