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- W38759991 abstract "Until recently, a major deficiency of most spectroscopic modeling of hot stars was the neglect of line-blanketing. With the availability of new atomic data, faster computers, suitable approximations, and improved numerical techniques it is now feasible to include non-LTE line-blanketing due to CNO and iron group elements in atmospheric calculations. We highlight the capabilities of the present generation of models. New blanketing results are presented for WN and WC Wolf-Rayet stars, and for LBVs. Line-blanketing alters individual line strengths in unpredictable ways, and can significantly influence the determination of stellar parameters. We specifically highlight the UV spectral region in which the effects of Fe blanketing are directly manifested. The importance of the charge exchange reaction Fe 2+ + H ⇌ Fe + + H + for modeling of the Fe emission lines in the extreme P-Cygni star HDE 316285 is illustrated." @default.
- W38759991 created "2016-06-24" @default.
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- W38759991 date "1999-01-01" @default.
- W38759991 modified "2023-09-25" @default.
- W38759991 title "Line-blanketing in massive stars: new results" @default.
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- W38759991 doi "https://doi.org/10.1017/s0074180900205238" @default.
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