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- W1977696593 abstract "Non-LTE line-formation calculations have been undertaken for Si II, Si III and Si IV ions using a new grid of model atmospheres. The principal difference to previous calculations is the completeness and reliability of the adopted atomic data. Equivalent widths of 58 silicon lines are presented for a range of effective temperatures (17500–30000K), logarithmic gravities (3.5–4.5), microturbulent velocities (0 and 5 km s−1) and silicon abundances (approximately 7.0–8.0 dex) appropriate to main-sequence early B-type stars. Also tabulated are the corresponding LTE line strengths. The importance of non-LTE effects, particularly in the near-infrared, are confirmed." @default.
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- W1977696593 date "1986-10-01" @default.
- W1977696593 modified "2023-09-25" @default.
- W1977696593 title "Non-LTE calculations of silicon-line strengths in B-type stars" @default.
- W1977696593 doi "https://doi.org/10.1093/mnras/222.4.719" @default.
- W1977696593 hasPublicationYear "1986" @default.
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