Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-01-28
Astronomy and Astrophysics
Astrophysics
13 pages, 3 figures; To appear in ApJ Letters
Scientific paper
10.1086/339471
Europium isotopic abundance fractions are reported for the very metal-poor, neutron-capture-rich giant stars CS 22892-052, HD 115444, and BD +17 3248. The abundance fractions, derived from analysis of several strong Eu II lines appearing in high-resolution spectra of these stars, are in excellent agreement with each other and with their values in the Solar System: fraction(\iso{Eu}{151}) ~= fraction(\iso{Eu}{153}) ~= 0.5. Detailed abundance studies of very metal-poor stars have previously shown that the total elemental abundances of stable atoms with atomic numbers z >= 56 typically match very closely those of a scaled solar-system r-process abundance distribution. The present results for the first time extend this agreement to the isotopic level.
Beers Timothy C.
Burles Scott
Cowan John J.
Fuller George M.
Lawler James E.
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