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Accuracy of Element Abundances from Stellar Atmospheres pp 57–67Cite as

The accuracy of abundances from middle B to F main sequence normal stars

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Part of the book series: Lecture Notes in Physics ((LNP,volume 356))

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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Author information

Authors and Affiliations

  1. Astronomical Institute, Osaka Kyoiku University, Tennoji-ku, 543, Osaka, Japan

    Kozo Sadakane

Authors
  1. Kozo Sadakane
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Editor information

Rainer Wehrse

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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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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-52365-9

  • Online ISBN: 978-3-540-46971-1

  • eBook Packages: Springer Book Archive

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