Volume 573, January 2015
|Number of page(s)||33|
|Published online||11 December 2014|
Lines retained in this analysis: atomic and solar data, line weightings, LTE abundance results for the 5 models used in this analysis, NLTE corrections to the LTE result (when available), and the corresponding 3D+NLTE abundance result.
HFS and isotopic splitting data for the lines retained in this analysis.
Our adopted ionisation energies Eion and partition functions U(T) for relevant ionisation stages of the iron group elements.
© ESO, 2014
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