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On the Precision of the MK Spectral Classification System

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Part of the book series: International Astronomical Union / Union Astronomique Internationale ((IAUS,volume 50))

Abstract

It is shown that a large scatter exists in all color-color and color-spectral type diagrams. This scatter can not be neglected and its importance is shown in several examples. A new approach is then developed for the study of the precision attainable in spectral classification. It is found that for A-type stars MK classification is about as accurate as photometry, whereas for B-type dwarfs photometry is at least two times more precise than MK classification. A precision of ±0.6 tenths of a spectral class seems attainable in both groups.

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Jaschek, C., Jaschek, M. (1973). On the Precision of the MK Spectral Classification System. In: Fehrenbach, C., Westerlund, B.E. (eds) Spectral Classification and Multicolour Photometry. International Astronomical Union / Union Astronomique Internationale, vol 50. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-2627-7_11

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  • DOI: https://doi.org/10.1007/978-94-010-2627-7_11

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-2629-1

  • Online ISBN: 978-94-010-2627-7

  • eBook Packages: Springer Book Archive

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