Neutron-Capture Element Trends in the Halo

Details Neutron-Capture Element Trends in the Halo Neutron-Capture Element Trends in the Halo

2001-01-24

arxiv.org/abs/astro-ph/0101439v1

Astronomy and Astrophysics

Astrophysics

6 pages, 2 figures. To appear in the Proceedings of ``Cosmic Evolution''

Scientific paper

In a brief review of abundances neutron-capture elements (Z > ~30) in
metal-poor halo stars, attention is called to their star-to-star scatter, the
dominance of r-process synthesis at lowest metallicities, the puzzle of the
lighter members of this element group, and the possibility of a better
r-/s-process discriminant.

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