Structure, Evolution, and Nucleosynthesis of Primordial Stars

  title={Structure, Evolution, and Nucleosynthesis of Primordial Stars},
  author={Lionel Siess and Mario Livio and John C. Lattanzio},
  journal={The Astrophysical Journal},
  pages={329 - 343}
The evolution of Population III stars (Z = 0) is followed from the pre-main-sequence phase up to the asymptotic giant branch (AGB) phase for intermediate-mass stars and up to C ignition in more massive stars. Our grid includes 11 stars, covering the mass range 0.8-20 M☉. During the H and He core burning phases an overshooting characterized by d = 0.20HP was applied, and during the AGB phase a small extension of the convective envelope was also allowed, characterized by d = 0.05HP. We find that… 
An explosive end to intermediate-mass zero-metallicity stars and early Universe nucleosynthesis
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On the mass of population III stars
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