Fig. 10
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Left panel: dependence of the N2/Ntot ratio on the present-day mass of MWGCs. Right panel: N2/Ntot ratio vs. the radius of the circular orbit. Colored dots indicate GC type, whether it formed in the MW or arrived with a dwarf galaxy absorbed by the MW: 0, black – in situ formation, 1, red – ex situ Gaia-Sausage/Enceladus formation, 2, blue – ex situ Sagittarius dwarf, 3, green – ex situ other mergers with dwarf galaxies, −1, purple – type not specified. Data are from catalogs: Milone et al. (2017); Bajkova & Bobylev (2021); Chen & Gnedin (2024); Baumgardt et al. (2019).
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