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>A high-resolution VLT/FLAMES study of individual stars in the centre of the Fornax dwarf spheroidal galaxy ( Corrigendum) ★
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A high-resolution VLT/FLAMES study of individual stars in the centre of the Fornax dwarf spheroidal galaxy ( Corrigendum) ★
Due to an unfortunate typo in Fortran I/O formats, incorrect values of the collisional broadening coefficient were passed to the spectral synthesis code (CALRAI) in our analysis of Fornax red giants stars. Furthermore, we realized that the lanthanum in tables and figures had escaped the HFS corrections described in Sect. 3.5 of the paper. Here we provide an updated table with all corrected abundances for 72 Fornax stars. The changes are small and non-systematic for most elements, except barium and lanthanum where they are more visible. We thus also reproduce here Figs. 8, 14, 16, and 20 which are the only figures with visible changes. All of our conclusions still hold, although for Ba and La, the overabundance with respect to the Milky Way are of a smaller magnitude than originally published.
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机译：由于Fortran I / O格式的错字，我们在分析Fornax红色巨星时将不正确的碰撞展宽系数值传递给了光谱综合码（CALRAI）。此外，我们意识到表和图中的镧已经摆脱了Sect中描述的HFS校正。 3.5篇论文。在这里，我们提供了更新的表格，其中包含72个Fornax星的所有校正后的丰度。对于大多数元素而言，这些变化很小且没有系统性，但钡和镧除外，这些元素更明显。因此，我们在这里也复制了图。图8、14、16和20是仅有的明显变化的数字。我们的所有结论仍然成立，尽管对于Ba和La来说，银河系的丰度比最初发表的要小。
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