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Classification of Stars with Different Chemical Constitution

Published online by Cambridge University Press:  14 August 2015

D. Chalonge  and
L. Divan
D. Chalonge
Affiliation:
Institut d'Astrophysique, Paris, France
L. Divan
Affiliation:
Institut d'Astrophysique, Paris, France

Abstract

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The possibility of obtaining a segregation between stars of different chemical constitution using the BCD classification is reviewed.

Type
Part IV/Abundance Effects in Spectral Classification
Information
Symposium - International Astronomical Union , Volume 72: Abundance Effects in Classification , 1976 , pp. 143 - 146
Copyright
Copyright © Reidel 1976 

References

Chalonge, D.: 1955, Principes Fondamentaux de Classification Stellaire , Colloques Internationaux du Centre National de la Recherche Scientifique, Paris, p. 55.Google Scholar
Chalonge, D.: 1966, in Lodén, K., Lodén, L. O. and Sinnerstad, U. (eds.), IAU Symp. 24, 77, Academic Press, London.Google Scholar
Chalonge, D. and Divan, L.: 1973, Astron. Astrophys. 23, 69.Google Scholar