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首页> 外文期刊>Astronomy and astrophysics >The odd-isotope fractions of barium in CEMP-r/s star HE 0338-3945 and r-II star CS 31082-001
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The odd-isotope fractions of barium in CEMP-r/s star HE 0338-3945 and r-II star CS 31082-001

机译:CEMP-r / s星HE 0338-3945和r-II星CS 31082-001中钡的奇数同位素分数

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摘要

We report the first measurement of the odd-isotope fractions for barium, f _(odd,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 f _(odd,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.
机译:我们报告了钡的奇数同位素分数f _(odd,Ba)的首次测量。在两个极贫金属的恒星中:CEMP- r / s恒星HE?0338-3945([Fe / H] =?2.42±0.11)和r -II恒星CS?31082-001([Fe / H] = 2.90±0.13)。测得的f _(odd,Ba)值是0.23±0.12,对应于HE?0338-3945的r过程贡献的34.3±34.3%,而0.43±0.09对应于ba的r过程贡献的91.4±25.7% CS?31082-001的生产。钡在CS?31082-001中的高r-处理特征(91.4±25.7%)表明该恒星中的大多数重元素是通过r-处理途径合成的,而较低的r-处理值(34.3± HE?0338-3945中发现的34.3%)表明该恒星中的重元素是通过s-过程和r-过程合成的混合而形成的。这些结论与基于渐近巨型分支星模型计算以适合其丰度分布的研究一致。

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