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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 13.

Mass fraction of H, He, C, N, O, and Ne as a function of the mass coordinate for the donor star (star 1) and the accreting star (star 2) in rotational binary model B2. Different evolutionary stages are indicated by the different colors: the beginning of the first episode of RLOF (red solid lines), the terminal of the first episode of RLOF (green dashed lines), the beginning of the second episode of RLOF (blue dotted lines), and the terminal of the second episode of RLOF (purple dashed–dotted lines.)

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