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Abundances in the Galactic Clusters of Hyades and M 67

Published online by Cambridge University Press:  14 August 2015

R. Foy
R. Foy*
Affiliation:
Observatoire de Meudon, France

Abstract

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Two Hyades dwarfs and two giants in the old galactic cluster M 67 have been carefully analyzed from 7 å mm−1 taken at OHP with an electronic camera. Measurements of weak lines lead to € the conclusion that both these clusters have a solar chemical composition, although they have very different ages.

Type
Part V/Abundances in Stellar Populations
Information
Symposium - International Astronomical Union , Volume 72: Abundance Effects in Classification , 1976 , pp. 209 - 212
Copyright
Copyright © Reidel 1976 

References

Blanc-Vaziaga, M.-J., Cayrel, G., and Cayrel, R.: 1973, Astrophys. J. 180, 871.CrossRefGoogle Scholar
Spinrad, H. and Taylor, D. J.: 1969, Astrophys. J. 157, 1279.CrossRefGoogle Scholar