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- W3102563669 abstract "Context.The knowledge of isotopic and elemental abundances of the pristine solar system material provides a fundamental test of galactic chemical evolution models, while the composition of the solar photosphere is a reference pattern to understand stellar abundances. However, spectroscopic or meteoritic abundance determinations are only possible for an incomplete sample of the 83 elements detected in the solar system. Therefore, only relative abundances are experimentally determined, with respect to or to for spectroscopic or meteoritic measurements, respectively. For this reason, the available compilations of solar abundances are obtained by combining spectroscopic and meteoritic determinations, a procedure requiring the knowledge of the chemical modification occurring in the solar photosphere." @default.
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- W3102563669 date "2006-11-21" @default.
- W3102563669 modified "2023-09-23" @default.
- W3102563669 title "A method to derive the absolute composition of the Sun, the solar system, and the stars" @default.
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- W3102563669 doi "https://doi.org/10.1051/0004-6361:20054505" @default.
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