Fig. 5.

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Left upper panel: distribution of cerium vs. metallicity for the low-uncertainty sample stars, colour-coded with the eccentricity of their orbits. Left lower panel: Toomre diagram colour-coded with [Ce/Fe]. The circular dashed lines corresponds to VTot = 50, 100 and 150 km s−1. Right panels: Energy-angular momentum (E, LZ) plane colour-coded by density (top panel), and medium cerium abundance (lower panel). The white star indicates the solar neighbourhood (LZ = L⊙, ).
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