Table 1.
Summary of the initial conditions employed in our simulations.
| NSPH | Mgas | Rgas | M1, gas | T | Nstar | Mstar | M1, star |
|---|---|---|---|---|---|---|---|
| [M⊙] | [pc] | [M⊙] | [K] | [M⊙] | [M⊙] | ||
| 218 | 3 × 104 | 0.14 | ∼0.11 | 500 | 256 | 25.6 | 0.1 |
| 218 | 3 × 104 | 0.14 | ∼0.11 | 1000 | 256 | 25.6 | 0.1 |
| 218 | 3 × 104 | 0.14 | ∼0.11 | 3000 | 256 | 25.6 | 0.1 |
| 218 | 3 × 104 | 0.14 | ∼0.11 | 5000 | 256 | 25.6 | 0.1 |
| 218 | 3 × 104 | 0.14 | ∼0.11 | 8000 | 256 | 25.6 | 0.1 |
Notes. We show the number of SPH particles used for each simulation. The input parameters are the initial gas mass Mgas, the initial gas radius Rgas, the approximate initial gas mass for each SPH particle M1, gas, the initial temperature T, the number of stars Nstars, the total stellar mass Mstar, and the mass of each star M1, star.
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