Wolf - Rayet Stars ∗


Wolf-Rayet (W-R) stars are a class of peculiar stars first identified in 1867 by C. J. E. Wolf and G. Rayet. Unlike the spectra of most stars, which are dominated by narrow absorption lines, the spectra of W-R stars show broad emission lines. The rich emission line spectrum makes them easy to identify, by spectroscopic observations, even at large distances… (More)


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@inproceedings{Stars2003WolfR, title={Wolf - Rayet Stars ∗}, author={Wolf-Rayet Stars and D. John Hillier}, year={2003} }