Fig. 9
[Ba/Y] ratio vs. [Fe/H] for H11 in magenta dots; Galactic data in black: dots from Fulbright (2000) and open circles from Nissen & Schuster (2011), blue squares are dSph data from Shetrone et al. (2001) and Shetrone et al. (2003), LMC data in red: triangles are J06, stars are old GCs from M10 and intermediate age clusters from Mucciarelli et al. (2008), open circles from Pompéia et al. (2008). The segmented line shows the Galactic trend.
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