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- W142499054 abstract "The Wolf-Rayet WO spectral sequence was introduced by Barlow & Hummer (1982) for four Pop I WR stars with very strong O VI 381 nm doublet emission. At the time, the evolution of very massive stars was poorly known, and their classification was based on phenomenological grounds. Recently, efforts to improve the WO spectral subtype classification are increasing (Kingsburgh et al. 1995; Crowther et al. 1998)." @default.
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- W142499054 date "1999-01-01" @default.
- W142499054 modified "2023-10-18" @default.
- W142499054 title "On the so-called WO stars" @default.
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- W142499054 doi "https://doi.org/10.1017/s0074180900205081" @default.
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