Abstract
The accuracy of abundance determinations of iron in middle B to F type stars is reviewed based on recent results. The relative importance of various sources of the error contained in observational data and in physical data is discussed.
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© 1990 Springer-Verlag
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Sadakane, K. (1990). The accuracy of abundances from middle B to F main sequence normal stars. In: Wehrse, R. (eds) Accuracy of Element Abundances from Stellar Atmospheres. Lecture Notes in Physics, vol 356. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0036064
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DOI: https://doi.org/10.1007/BFb0036064
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