Fig. 1.

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Distribution of the general populations of (left) UDGs, (middle) LSBs, and (right) dIrrs in the space of their defining physical parameters: μg, 0 − Re, μB, 0, and MV, respectively. In each case, we denote the sample galaxies used for constructing dynamical models in black. The dotted lines indicate the ranges of respective parameters allowed for these galaxy classes.
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