MODELING THE POLLUTION OF PRISTINE GAS IN THE EARLY UNIVERSE

@article{Pan2013MODELINGTP,
  title={MODELING THE POLLUTION OF PRISTINE GAS IN THE EARLY UNIVERSE},
  author={Liubin Pan and Evan Scannapieco and John Michael Scalo},
  journal={The Astrophysical Journal},
  year={2013},
  volume={775}
}
We conduct a comprehensive theoretical and numerical investigation of the pollution of pristine gas in turbulent flows, designed to provide useful new tools for modeling the evolution of the first generation of stars. The properties of such Population III (Pop III) stars are thought to be very different than those of later stellar generations, because cooling is dramatically different in gas with a metallicity below a critical value Zc, which lies between ∼10−6 and ∼10−3 Z☉. The critical value… 
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