Enrichment of the heaviest elements Th and Pb in the Galaxy

Details Enrichment of the heaviest elements Th and Pb in the Galaxy Enrichment of the heaviest elements Th and Pb in the Galaxy

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aps..haw1wc001a&link_type=abstract

American Physical Society, 3rd Joint Meeting of the APS Division of Nuclear Physics and the Physical Society of Japan, October 1

Physics

Nuclear Physics

Scientific paper

The heaviest elements Th and Pb are key to understanding the neutron-capture reactions in the Universe. Abundance measurements of these elements for metal-deficient stars in the past dacade provide useful constraints on both the r- and s-processes, and early chemical enrichment in the Galaxy. Recent observational results on abundance ratios of Th to other stable elements in metal-deficient stars, Pb production of both r- and s-processes, and their enrichment history in the Galaxy are reviewed.

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