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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 1.

(a) Convective core for nonrotating single stars with different convective criteria as a function of evolutionary ages. (b) Convective core for single stars with different various metallicities and rotational velocities as a function of evolutionary ages. (c) Convective core for the donor star (solid lines) and the accreting star (dashed lines) in the binary system with differential orbital period as a function of evolutionary ages. (d) Convective core for two components in the binary system with different metallicities and stellar mass as a function of evolutionary ages.

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