Low-metallicity massive single stars with rotation. Evolutionary models applicable to I Zwicky 18

@article{Szecsi2015LowmetallicityMS,
  title={Low-metallicity massive single stars with rotation. Evolutionary models applicable to I Zwicky 18},
  author={Dorottya Sz'ecsi and Norbert Langer and S.-C. Yoon and D. Sanyal and Selma E. de Mink and C. J. Evans and Tyl Dermine},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2015}
}
Massive rotating single stars with an initial metal composition appropriate for the dwarf galaxy I Zw 18 ([Fe/H]=$-$1.7) are modelled during hydrogen burning for initial masses of 9-300 M$_{\odot}$ and rotational velocities of 0-900 km s$^{-1}$. Internal mixing processes in these models were calibrated based on an observed sample of OB-type stars in the Magellanic Clouds. Even moderately fast rotators, which may be abundant at this metallicity, are found to undergo efficient mixing induced by… 

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