Determination of Surface Abundances for HD 129174 (π 1 Boo)

Richard Monier
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Abstract

The synthesis of the Hg ii line at 3983.93 Å, using published hyperfine structure and nuclear shifts, confirms a large overabundance of mercury in HD 129174, about +6.18 dex, which is actually slightly larger than the excess derived in earlier studies. The synthesis of 17 other lines close to the Hg ii line and in the spectral range 4400–4500 Å yields abundances for 9 elements. Helium and iron are found to be deficient by −1.12 and −0.097 dex. Magnesium, scandium, titanium, chromium are moderately enhanced by respectively +0.30 dex (Mg) and +1.0 dex (Sc, Ti and Cr). Yttrium and zirconium are very overabundant by +4.00, +2.48 dex respectively.
测定 HD 129174 的表面丰度(π 1 Boo)
利用已公布的超频结构和核移位,对 3983.93 Å 处的 Hg ii 线进行合成,证实 HD 129174 中的汞大量过剩,约为 +6.18 dex,实际上比早期研究得出的过剩量稍大。对靠近 Hg ii 线和 4400-4500 Å 光谱范围内的 17 条其他线的综合分析得出了 9 种元素的丰度。发现氦和铁分别缺乏-1.12 和-0.097 dex。镁、钪、钛、铬的丰度分别为+0.30 dex(镁)和+1.0 dex(钪、钛和铬)。钇和锆的含量非常高,分别为 +4.00 和 +2.48 dex。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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