We report the first measurement of the odd-isotope fractions for barium, fodd,Ba in two extremely metal-poor stars: a CEMP-r/s star HE 0338-3945 ([Fe/H] =-2.42 ± 0.11) and an r-II star CS 31082-001 ([Fe/H] =-2.90 ± 0.13). The measured fodd,Ba values are 0.23 ± 0.12 corresponding to 34.3 ± 34.3% of the r-process contributions for HE 0338-3945 and 0.43 ± 0.09 corresponding to 91.4 ± 25.7% of the r-process contribution to Ba production for CS 31082-001. The high r-process signature of barium in CS 31082-001 (91.4 ± 25.7%) suggests that the majority of the heavy elements in this star were synthesised via an r-process path, while the lower r-process value (34.3 ± 34.3%) found in HE 0338-3945 indicates that the heavy elements in this star formed through a mix of s-process and r-process synthesis. These conclusions are consistent with studies based on asymptotic giant branch star model calculations to fit their abundance distributions.
CITATION STYLE
Meng, X. Y., Cui, W. Y., Shi, J. R., Jiang, X. H., Zhao, G., Zhang, B., & Li, J. (2016). The odd-isotope fractions of barium in CEMP-r/s star HE 0338-3945 and r-II star CS 31082-001. Astronomy and Astrophysics, 593. https://doi.org/10.1051/0004-6361/201527318
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