No CrossRef data available.
Article contents
[Fe/H] Ratios in Population II Stars
Published online by Cambridge University Press: 19 July 2016
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.
Abundances of Population II stars of the field and globular cluster systems are reviewed. Emphasis is placed on [Fe/H] ratios determined from analyses of moderate- and high-resolution spectroscopic data. The status of analyses of metal-deficient stars is examined from the viewpoint of number of analyses and number of stars, overall distribution of the [Fe/H] ratios, and systematics of the [Fe/H] ratios.
- Type
- The Giants
- Information
- Copyright
- Copyright © Kluwer 1991
References
Cayrel de Strobel, G., Bentolila, C., Hauck, B., and Duguennoy, A.
1985,
Astr. Ap. Suppl.
59, 145.Google Scholar
Cayrel de Strobel, G., Spite, M., and Lloyd Evans, T., (eds.) 1988,
The abundance spread within Globular Clusters: spectroscopy of individual stars
(IAU JCM 5 and CM37/3), Paris Observatory, Paris.Google Scholar