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Spectral Classification from a Theoretical Point of View

Published online by Cambridge University Press:  12 April 2016

Erika Bohm-Vitense*
Affiliation:
University of Washington

Abstract

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We study the conditions under which a two-dimensional spectral classification according to Teff and ne is possible and when 3- or It-dimensional spectral classification is necessary because the classification criteria are unavoidably influenced by the metal and helium abundances. For late type stars, where molecular absorption becomes important for the continuum a seven-or more- dimensional classification may be necessary. At this point spectral classification may not be useful any more. We find generally that a derivation of the gravitational acceleration from the spectroscopically determined electron density is only possible if the helium abundance is known.

Type
VII Theoretically and Empirically Oriented Approach to Spectral Classification
Copyright
Copyright © Vatican Observatory 1979

References

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