Fig. 6
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[Mg/Fe] − [Al/Fe] distribution for HP 1 stars (cyan symbols). The black “X” symbol show the average [Mg/Fe] and [Al/Fe] abundance ratios of HP 1 from our BACCHUS values listed in Table 3. The dashed black line taken from Belokurov & Kravtsov (2024) separates the region dominated by in situ GCs (above the line) from accreted GCs (below the line).
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