Elemental and isotopic abundances in metal-deficient stars

Details Elemental and isotopic abundances in metal-deficient stars Elemental and isotopic abundances in metal-deficient stars

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005nupha.758..209a&link_type=abstract

Nuclear Physics A, Vol. 758, p.209-216

Physics

Nuclear Physics

1

Scientific paper

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.

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