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- W1617456156 abstract "Abstract Over the last half-century quantitative stellar spectroscopy has made great progress. However, most stellar abundance analyses today still employ rather simplified models, which can introduce severe systematic errors swamping the observational errors. Some of these uncertainties for late-type stars are briefly reviewed here: atomic and molecular data, stellar parameters, model atmospheres and spectral line formation." @default.
- W1617456156 created "2016-06-24" @default.
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- W1617456156 date "2005-01-01" @default.
- W1617456156 modified "2023-10-16" @default.
- W1617456156 title "Uncertainties in Stellar Abundance Analyses" @default.
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- W1617456156 doi "https://doi.org/10.1017/s1539299600016555" @default.
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