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- W583382015 abstract "We want to include the opacity of millions or hundreds of millions of lines in model stellar atmosphere calculations, then generate detailed, realistic spectra from those model atmospheres, then model the observation process, and finally compare the calculated spectra to observed spectra to determine the properties of stars so that we can understand their evolution and the evolution of galaxies." @default.
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- W583382015 date "2014-01-01" @default.
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- W583382015 title "How to Build a Model of the Atmosphere and Spectrum" @default.
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- W583382015 doi "https://doi.org/10.1007/978-3-319-06956-2_3" @default.
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