Total nucleosynthetic yields for selected isotopes in solar masses for our 150 M⊙ and 250 M⊙ models (including matter lost by stellar wind and decay products) in comparison with 70 M⊙ and 115 M⊙ zero metallicity helium star yields (Heger & Woosley 2002), respectively.
|He 70 M⊙||0||–||1.5||4.5||45.8||4.0||3.0||8.0||2.4||0.3||0.2||10-4||10-4||0.01|
|He 115 M⊙||0||–||1.8||3.7||40.||3.8||4.5||25.7||11.8||1.9||1.6||10-5||10-4||19.0|
Notes. Yields for hydrogen and helium neglecting the wind matter are given after the slash sign.
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