| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 9850945 | Nuclear Physics A | 2005 | 8 Pages |
Abstract
Recent observational studies of metal-deficient stars using large telescopes have revealed the elemental abundances for a wide range of atomic (mass) number for neutron-capture elements (31⩽Z⩽92), and also isotopic abundance ratios for several elements (e.g., Li, Mg, Eu). In this paper we review these recent studies, in particular the abundance pattern of light neutron-capture elements (Sr-Pd) and the Eu isotope ratios produced by the s-process.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
W. Aoki,