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Abundances in the Galactic Clusters of Hyades and M 67
Published online by Cambridge University Press: 14 August 2015
Abstract
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
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