Fig. C.1.
Relation between the potential and kinetic energy for all TDGCs of sample A. The colorbar presents the stellar mass, Mstellar, of the TDGCs. The black solid lines highlight the condition for virial equilibrium, i.e., where the virial ratio becomes q = 1 (see Eq. (C.1)). All objects above the black dashed line are gravitationally bound (q < 2).
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