• Corpus ID: 18261125

Are peculiar Wolf-Rayet Stars of type WN8 Thorne-Zytkow Objects?

@article{Foellmi2002ArePW,
  title={Are peculiar Wolf-Rayet Stars of type WN8 Thorne-Zytkow Objects?},
  author={C'edric Foellmi and Anthony F. J. Moffat},
  journal={arXiv: Astrophysics},
  year={2002}
}
Most population I Wolf-Rayet (WR) stars are the He-rich descendants of the most massive stars (M_i = 25 - 100 M_sun). Evidence has been accumulating over the years that among all pop I WR stars, those of the relatively cool, N-rich subtype "WN8" are among the most peculiar: 1. They tend to be runaways, with large space velocity and/or avoid clusters. 2. Unlike their equally luminous WN6,7 cousins, only a very small number of WN8 stars are known to belong to a close binary with an OB companion… 

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