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Spectroscopic Criteria for the Classification of Peculiar B-type Stars with Colour-Spectrum Discrepancies
Published online by Cambridge University Press: 14 August 2015
Abstract
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The so-called ‘weak helium’ stars are discussed from a spectral classification point of view. Several authors have included different kinds of objects in this class. Often, the only similarity is the discrepancy between the spectra and the colours. It is desirable to decouple the discovery of new members of the class from this dependence on colours so that the colour can be used as an independent parameter.
- Type
- Part I: Classification of Slit Spectra
- Information
- Copyright
- Copyright © Reidel 1973
References
Klinglesmith, D. A., Bernacca, P. L., and Frey, H.: 1971, Bamberg Conference on Variable Stars, Veroeffentl. Remeis-Sternwarte Bamberg
9, Nr. 100, p. 205.Google Scholar
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