Fig. 5
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[Mg/Fe] versus [Fe/H], The stars in this work are presented as stellar markers, while other stars from Mackereth et al. (2021) are represented as teal dots (from GALAH DR3 data). We also show as black contour lines the kernel density estimate of metal-poor stars with retrograde motion from GALAH DR3 survey. The stars presented in this work are color-coded according to BASTA seismic stellar ages.
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