Table 2.
Overview of the simulations reported in this work and simulation parameters.
Simulation | Zinit (Z⊙) | mgas (M⊙) | m⋆ (M⊙) | mDM (M⊙) | ϵgas, max (pc) | ϵ⋆ (pc) | ϵDM (pc) | Feedback channels |
---|---|---|---|---|---|---|---|---|
0.02 Z⊙/full | 0.02 | 1 | 1 | 2.5 × 103 | 0.05 | 0.05 | 39 | PI+RP+PE+WD+SN |
0.02 Z⊙/full/low | 0.02 | 10 | 10 | 2.5 × 104 | 0.3 | 0.3 | 84 | PI+RP+PE+WD+SN |
0.02 Z⊙/noRT | 0.02 | 1 | 1 | 2.5 × 103 | 0.05 | 0.05 | 39 | WD+SN |
0.02 Z⊙/noRT/low | 0.02 | 10 | 10 | 2.5 × 104 | 0.3 | 0.3 | 84 | WD+SN |
0.2 Z⊙/full | 0.2 | 1 | 1 | 2.5 × 103 | 0.05 | 0.05 | 39 | PI+RP+PE+WD+SN |
0.2 Z⊙/full/low | 0.2 | 10 | 10 | 2.5 × 104 | 0.3 | 0.3 | 84 | PI+RP+PE+WD+SN |
Notes. The columns from left to right are the model name (first column), initial metallicity (second column), target mass of gas particles (third column), mass of star particles (both background and active stars, fourth column), mass of dark matter particles (fifth column), max softening length of gas (sixth column), softening length of stars (seventh column) and DM (eighth column), and the stellar feedback channels included in the models (ninth column). Abbreviations: PI: photoionization, RP: radiation pressure, PE: photoelectric heating, WD: stellar wind, SN: supernova.
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