Fig. 5.
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Projected Ω vs. i orbital solutions for the three young stars that have known orbital elements that correspond to a known GC disk feature (within error bars). All features are marked here by ellipses (see, e.g., Bartko et al. 2009; Yelda et al. 2014; von Fellenberg et al. 2022). Disk features are as calculated for Fig. 7 of von Fellenberg et al. (2022; hereafter, vF22).
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