Hostname: page-component-77c89778f8-n9wrp Total loading time: 0 Render date: 2024-07-18T01:24:17.291Z Has data issue: false hasContentIssue false
  • English
  • Français

[Fe/H] Ratios in Population II Stars

Published online by Cambridge University Press:  19 July 2016

R. Earle Luck
R. Earle Luck*
Affiliation:
Department of Astronomy Case Western Reserve University Cleveland, OH 44106 USA

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
Symposium - International Astronomical Union , Volume 145: Evolution of Stars: The Photospheric Abundance Connection , 1991 , pp. 247 - 256
Copyright
Copyright © Kluwer 1991 

References

Abia, C., and Rebolo, R. 1989, Ap. J. 347, 186.CrossRefGoogle Scholar
Caldwell, S. P., and Dickens, R. J. 1988, M. N. R. A. S. 233, 367.CrossRefGoogle Scholar
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
Gustafsson, B., Bell, R. A., Eriksson, K., and Nordlund, A. 1975, Astr. Ap., 42, 407.Google Scholar
Gratton, R. G. 1987 Astr. Ap. 179, 181.Google Scholar
Gratton, R. G. 1989 Astr. Ap. 211, 41.Google Scholar
Paltoglou, G., and Norris, J. E. 1989, Ap. J. 336, 185.CrossRefGoogle Scholar
Pilachowski, C. A. 1984, Ap. J. 281, 614.CrossRefGoogle Scholar
Spite, M., and Spite, F. 1985, A.R.A.A. 23, 225.Google Scholar
Wheeler, J. C., Sneden, C., and Truran, J. W. 1989, A.R.A.A. 27, 279.Google Scholar