Fig. 11
[La/Eu] from Johnson et al. (2012) and Van der Swaelmen et al. (2016; pink and blue larger symbols, respectively) of bulge stars compared to data from Battistini & Bensby (2016; triangles), Mishenina et al. (2013; squares), and Ishigaki et al. (2013; diamonds) for solar vicinity stars. There is no evidence from this data that the bulge and the solar vicinity distributions are different.
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