On the Role of Continuum-driven Eruptions in the Evolution of Very Massive Stars and Population III Stars

@article{Smith2006OnTR,
  title={On the Role of Continuum-driven Eruptions in the Evolution of Very Massive Stars and Population III Stars},
  author={Nathan Smith and Stanley P. Owocki},
  journal={The Astrophysical Journal Letters},
  year={2006},
  volume={645},
  pages={L45 - L48}
}
We suggest that the mass lost during the evolution of very massive stars may be dominated by optically thick, continuum-driven outbursts or explosions, instead of by steady line-driven winds. In order for a massive star to become a Wolf-Rayet star, it must shed its hydrogen envelope, but new estimates of the effects of clumping in winds from O-type stars indicate that line driving is vastly insufficient. We discuss massive stars above roughly 40-50 M☉, which do not become red supergiants and… 

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