Table 7.
Medians of simulated stellar half-mass radii, R0.5 stellar, for dispersion-dominated (κrot < 0.5) DMC stellar objects, DMC DGs, and TDGCs samples for different stellar mass ranges.
| Sample | Mdm/Mbaryonic | Mstellar [M⊙]: | 107−108 | 108−109 | 109−1010 | 1010−1011 | 1011−1012 |
|---|---|---|---|---|---|---|---|
| DMC stellar objects | >0 | ⟨R0.5 stellar⟩ [pc]: | 4342 | 5770 | 7232 | 8213 | 11 697 |
| DM-rich stellar objects | ≥1 | 4346 | 5779 | 7246 | 8235 | 11 717 | |
| DM-poor stellar objects | <1 | 1903 | 1681 | 1687 | 3994 | 3445 | |
| DMC DGs | >0 | 4633 | 582 | – | – | – | |
| DM-rich DGs | ≥1 | 4635 | 5826 | – | – | – | |
| DM-poor DGs | <1 | 2667 | 2185 | – | – | – | |
| TDGCs | 0 | 1657 | 1125 | 773 | – | – | |
| Observed | – | ⟨R0.5 light⟩ [pc]: | 969 | 1339 | 1988 | 3930 | 8315 |
Notes. The medians of the 3D deprojected half-light radii, R0.5 light, of observed early type galaxies for different stellar mass ranges are given in the last row (Dabringhausen & Fellhauer 2016). The statistical properties of simulated and observed galaxies are visualized in Fig. 14.
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