Fig. 20
[La/Fe] ratios as a function of [Eu/Fe] ratios for individual stars in M 80 (large filled circles) compared to r-only field stars from Roederer et al. (2010; small empty squares) and to a GC with a dispersion in r-process from Roederer (2011): M 15 (filled triangles), with abundances from Otsuki et al. (2006) and Sobeck et al. (2011). The internal error bars refer to our analysis of M 80.
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