Gas (green), stellar (red), and dark matter (black) mass evolution of TDGCs and DM-poor objects shown in Fig. 2 starting from the first time step at which the first stellar particles in their subhalos appeared. Their ID numbers are given in the upper-right corner of the panels and the discussed subhalos of each row belong to the same host galaxy. The subhalo ID 404879 has M_stellar = 2.2 × 10⁷ M_⊙, M_gas = 3.0 × 10⁸ M_⊙, and M_dm = 6.3 × 10⁶ M_⊙ and is thus not included in the main sample of DMC (-poor) DGs (see Table 2). The dashed and long-dashed horizontal lines indicate the initial baryonic (1.26 × 10⁶ M_⊙) and dark matter mass (6.26 × 10⁶ M_⊙) of a particle. The dark matter content is short lived and is due to individual dark matter particles crossing the objects.