Table 1.
Main properties of the simulated galaxies used in this work.
| ID | Mhalo | M* | MH I | SFR |
|---|---|---|---|---|
| [1012 M⊙] | [1010 M⊙] | [1010 M⊙] | [M⊙ yr−1] | |
| 520885 | 1.17 | 5.47 | 3.17 | 2.76 |
| 555013 | 0.89 | 3.66 | 1.85 | 1.48 |
Notes. The galaxies are part of the TNG50 Milky Way-like sample provided by Ramesh et al. (2023) and the HI properties has been derived by Marasco et al. (in prep). The ID refers to the subhalo index in the group catalogues as determined by the subfind algorithm (Dolag et al. 2009). Mhalo, M* and MH I are the dark matter halo, stellar and HI masses, respectively. SFR is the current star formation rate.
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