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In a brief review of abundances neutron-capture elements (Z > ~30) inmetal-poor halo stars, attention is called to their star-to-star scatter, thedominance of r-process synthesis at lowest metallicities, the puzzle of thelighter members of this element group, and the possibility of a betterr-/s-process discriminant.Comment: 6 pages, 2 figures. To appear in the Proceedings of ``Cosmic  Evolution'

NEUTRON-CAPTURE ELEMENT TRENDS IN THE HALO