Spectral analysis and model atmospheres of WR type central stars

@article{Hamann1996SpectralAA,
  title={Spectral analysis and model atmospheres of WR type central stars},
  author={W. R. Hamann},
  journal={Astrophysics and Space Science},
  year={1996},
  volume={238},
  pages={31-42}
}
  • W. Hamann
  • Published 1 April 1996
  • Physics
  • Astrophysics and Space Science
Wolf-Rayet type spectra of central stars are compared with spectra from Pop. I objects. Non-LTE models for expanding atmospheres are applied for analyzing these spectra quantitatively. 

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