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Fig. 14


Solar r-process abundance values. Top: deconvolution from Simmerer et al. (2004) scaled to Eu (solid line) compared with the new observed abundances in CS 31082-001 (black dots and respective error bars). Radioactive element (Th and U) abundances are corrected for radioactive decay since the formation of the solar system. The dotted line shows the abundances observed today for these two species. Bottom: abundance residuals. NLTE abundances for some elements (red dots and respective error bars) are compared with the LTE results. For Pb, the green symbol represents the NLTE+3D corrected value.

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