Table 3
Details of the performed simulations.
| # | Size | Tdust | Mfilam |  |
n0 | B0 | B-field | OPR(H2) | ⟨a⟩ |
|---|---|---|---|---|---|---|---|---|---|
| Core | (pc) | (K) | (M⊙) | (cm−3) | (μG) | [μm] | |||
| F1_0035 | 1.6 | 15 | 120 | 5 | 7.6 × 104 | 40 | ∥ | 0.1 | 0.035 |
| F1_0035_OPR | 1.6 | 15 | 120 | 5 | 7.6 × 104 | 40 | ∥ | 0.001 | 0.035 |
| F1_01 | 1.6 | 15 | 120 | 5 | 7.6 × 104 | 40 | ∥ | 0.1 | 0.1 |
| F2_01 | 1.6 | 10 | 80 | 1 | 5.0 × 104 | 40 | ∥ | 0.1 | 0.1 |
| F3_01 | 1.6 | 10 | 80 | 1 | 5.0 × 104 | 40 | ⊥ | 0.1 | 0.1 |
Notes. We report the filament size, dust temperature, the filament mass Mfilam, the Mach number
, filament central density n0, initial magnetic field strength B0, and the initial chemical parameters: H2 ortho-to-para ratio and average grain size, ⟨a⟩. We set the instability parameter 
for all the runs, with 
, cs the thermal sound speed and G the gravitational constant. We note that in our isothermal simulations, we assumed Tdust = Tgas.
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