No CrossRef data available.
Article contents
Can We Check by High-Dispersion Analyses Stars Belonging to Eggen's Moving Groups?
Published online by Cambridge University Press: 14 August 2015
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
We describe the results of analysis of the giant star HD 6497, which belongs to the Arcturus group.
- Type
- Part IV/Abundance Effects in Spectral Classification
- Information
- Symposium - International Astronomical Union , Volume 72: Abundance Effects in Classification , 1976 , pp. 173 - 175
- Copyright
- Copyright © Reidel 1976
References
Mäckle, R., Holweger, H., Griffin, R. and Griffin, R.: 1975,
Astron. Astrophys.
38, 239.Google Scholar
You have
Access