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Table 3.
Comparison of the initial conditions of the GLMC, GSMC, and GMW galaxies for the fiducial model presented in this work (KRATOS) and the model presented by Besla et al. (2012, B12).
| KRATOS | B12 | |
|---|---|---|
| (Pure N-body) | (Hydrodynam.) | |
| [GLMC] | ||
| Stellar Distribution | Disc | Disc |
| Scale Length (kpc) | 2.85 | 1.7 |
| Scale Height (kpc) | 0.20 | 0.34 |
| Stellar Mass (M⊙) | 5.0 × 109 | 2.5 × 109 |
| DM Distribution | NFW | Hernquist |
| DM Concentration | 9 | 9 |
| DM Mass (M⊙) | 1.8 × 1011 | 1.8 × 1011 |
| [GSMC] | ||
| Stellar Distribution | NFW | Disc |
| Stellar Mass (M⊙) | 2.6 × 108 | 2.6 × 108 |
| DM Distribution | NFW | Hernquist |
| DM Concentration | 15 | 15 |
| DM Mass (M⊙) | 1.9 × 1010 | 2.1 × 1010 |
| [GMW] | ||
| DM Distribution | NFW | Static NFW |
| DM Concentration | 12 | 12 |
| DM Mass (M⊙) | 1.0 × 1012 | 1.5 × 1012 |
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