Fig. 11.

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Kernel density estimation models of the characteristic orbital energy ((Emax + Emin)/2), the orbital Jacobi energy (EJ), orbital pericentre and apocentre, orbital eccentricity, and maximum vertical height above the Galactic plane for GCs with an Galactic origin (e.g., Massari et al. 2019). The position of FSR 1776 is shown as a black dot.
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