Fig. 8

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Distribution of stars selected from GALAH DR4 in the following elemental abundance planes: (a) [Mg/Fe] − [Fe/H], (b) [Ba/Fe] − [Fe/H], (c) [Ba/Mg] − [Fe/H]. The gray dots represent the total sample, while the colored lines show running means with shaded error regions for stars from kinematic structures as labeled in the legend. Stars in Thamnos2 are shown as dots due to the low number of stars in the group. The dashed lines indicate where the x- and y-axis are equal to zero.
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