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• W2057665305 abstract "Spectroscopy is the most powerful tool in astrophysics. One obtains information on stellar structure, temperature, gravity, chemistry, and age by means of analysis of spectral observations. Accurate determination of all these parameters depends on an adequate response from laboratory and theoretical spectroscopy. We consider the contribution of different parameters of atomic and molecular lines to stellar atmospheric and abundance analysis. The role of completeness of atomic and molecular data is emphasized." @default.
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• W2057665305 date "2014-11-01" @default.
• W2057665305 modified "2023-10-18" @default.
• W2057665305 title "The role of atomic and molecular data in stellar atmosphere studies: atmospheric structure and chemistry" @default.
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• W2057665305 doi "https://doi.org/10.1088/0031-8949/89/11/114007" @default.
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