| Model . | |$L\, (\mathrm{pc})$| . | |$\rho _0\, (\mathrm{g\, cm^{-3}})$| . | |$M_{\mathrm{cl}}\, (\mathrm{M_\odot })$| . | |$M_{\mathrm{cl}}/M_{\mathrm{J}}$| . | |$\mathcal {M}$| . | |$B_0\, (\mathrm{\mu G})$| . | |$\mathcal {M_{\mathrm{A}}}$| . | |$\mu _{\mathrm{B}}$| . | |$\beta$| . | |$N_{\mathrm{sims}}$| . | |$N_{\mathrm{tot}}$| . | |$\overline{M}_{\mathrm{median}}\, (\mathrm{M_\odot })$| . | |$\overline{M}_{\mathrm{average}}\, (\mathrm{M_\odot })$| . | |$\overline{M}_{50}\, (\mathrm{M_\odot })$| . |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . | (9) . | (10) . | (11) . | (12) . | (13) . | (14) . | (15) . |
| |$\alpha _{\mathrm{vir}}= 0.0625$| | 2 | |$5.25\times 10^{-20}$| | 6200 | 2091.0 | 5 | 10 | 2.9 | 19.7 | 0.7 | 1 | 517 | |$0.25\pm 0.02$| | |$0.50\pm 0.05$| | |$1.04\pm 0.19$| |
| |$\alpha _{\mathrm{vir}}= 0.125$| | 2 | |$2.62\times 10^{-20}$| | 3100 | 737.1 | 5 | 28 | 2.9 | 13.7 | 0.7 | 2 | 520 | |$0.27\pm 0.05$| | |$0.46\pm 0.08$| | |$0.93\pm 0.15$| |
| |$\alpha _{\mathrm{vir}}= 0.5$| | 2 | |$6.56\times 10^{-21}$| | 775 | 92.4 | 5 | 20 | 2.9 | 6.9 | 0.7 | 10 | 449 | |$0.46\pm 0.06$| | |$0.73\pm 0.08$| | |$1.38\pm 0.16$| |
| Model . | |$L\, (\mathrm{pc})$| . | |$\rho _0\, (\mathrm{g\, cm^{-3}})$| . | |$M_{\mathrm{cl}}\, (\mathrm{M_\odot })$| . | |$M_{\mathrm{cl}}/M_{\mathrm{J}}$| . | |$\mathcal {M}$| . | |$B_0\, (\mathrm{\mu G})$| . | |$\mathcal {M_{\mathrm{A}}}$| . | |$\mu _{\mathrm{B}}$| . | |$\beta$| . | |$N_{\mathrm{sims}}$| . | |$N_{\mathrm{tot}}$| . | |$\overline{M}_{\mathrm{median}}\, (\mathrm{M_\odot })$| . | |$\overline{M}_{\mathrm{average}}\, (\mathrm{M_\odot })$| . | |$\overline{M}_{50}\, (\mathrm{M_\odot })$| . |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . | (9) . | (10) . | (11) . | (12) . | (13) . | (14) . | (15) . |
| |$\alpha _{\mathrm{vir}}= 0.0625$| | 2 | |$5.25\times 10^{-20}$| | 6200 | 2091.0 | 5 | 10 | 2.9 | 19.7 | 0.7 | 1 | 517 | |$0.25\pm 0.02$| | |$0.50\pm 0.05$| | |$1.04\pm 0.19$| |
| |$\alpha _{\mathrm{vir}}= 0.125$| | 2 | |$2.62\times 10^{-20}$| | 3100 | 737.1 | 5 | 28 | 2.9 | 13.7 | 0.7 | 2 | 520 | |$0.27\pm 0.05$| | |$0.46\pm 0.08$| | |$0.93\pm 0.15$| |
| |$\alpha _{\mathrm{vir}}= 0.5$| | 2 | |$6.56\times 10^{-21}$| | 775 | 92.4 | 5 | 20 | 2.9 | 6.9 | 0.7 | 10 | 449 | |$0.46\pm 0.06$| | |$0.73\pm 0.08$| | |$1.38\pm 0.16$| |
Note. Column 1: MHD simulation models with different virial parameter |$\alpha _{\mathrm{vir}}$|. Column 2: size of the cloud/computational domain. Columns 3: initial mean gas density. Column 4: total mass of the cloud. Columns 5: number of Jeans masses in the cloud. Column 6: rms sonic Mach number. Column 7: initial magnetic field strength. Column 8: Alfv|$\acute{\text{e}}$|n Mach number. Column 9: mass-to-flux ratio. Column 10: plasma beta (thermal-to-magnetic pressure ratio). Column 11: number of simulations (random seeds for the turbulence driving) performed. Column 12: total number of sink particles formed. Column 13: median stellar mass. Column 14: mean stellar mass. Column 15: |$M_{\mathrm{50}}$|, which is the median mass in a cumulative mass function. Quantities in Columns (13)–(15) are averaged over the SFE range |$1-5~{{\ \rm per\ cent}}$| (represented by overbars).
| Model . | |$L\, (\mathrm{pc})$| . | |$\rho _0\, (\mathrm{g\, cm^{-3}})$| . | |$M_{\mathrm{cl}}\, (\mathrm{M_\odot })$| . | |$M_{\mathrm{cl}}/M_{\mathrm{J}}$| . | |$\mathcal {M}$| . | |$B_0\, (\mathrm{\mu G})$| . | |$\mathcal {M_{\mathrm{A}}}$| . | |$\mu _{\mathrm{B}}$| . | |$\beta$| . | |$N_{\mathrm{sims}}$| . | |$N_{\mathrm{tot}}$| . | |$\overline{M}_{\mathrm{median}}\, (\mathrm{M_\odot })$| . | |$\overline{M}_{\mathrm{average}}\, (\mathrm{M_\odot })$| . | |$\overline{M}_{50}\, (\mathrm{M_\odot })$| . |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . | (9) . | (10) . | (11) . | (12) . | (13) . | (14) . | (15) . |
| |$\alpha _{\mathrm{vir}}= 0.0625$| | 2 | |$5.25\times 10^{-20}$| | 6200 | 2091.0 | 5 | 10 | 2.9 | 19.7 | 0.7 | 1 | 517 | |$0.25\pm 0.02$| | |$0.50\pm 0.05$| | |$1.04\pm 0.19$| |
| |$\alpha _{\mathrm{vir}}= 0.125$| | 2 | |$2.62\times 10^{-20}$| | 3100 | 737.1 | 5 | 28 | 2.9 | 13.7 | 0.7 | 2 | 520 | |$0.27\pm 0.05$| | |$0.46\pm 0.08$| | |$0.93\pm 0.15$| |
| |$\alpha _{\mathrm{vir}}= 0.5$| | 2 | |$6.56\times 10^{-21}$| | 775 | 92.4 | 5 | 20 | 2.9 | 6.9 | 0.7 | 10 | 449 | |$0.46\pm 0.06$| | |$0.73\pm 0.08$| | |$1.38\pm 0.16$| |
| Model . | |$L\, (\mathrm{pc})$| . | |$\rho _0\, (\mathrm{g\, cm^{-3}})$| . | |$M_{\mathrm{cl}}\, (\mathrm{M_\odot })$| . | |$M_{\mathrm{cl}}/M_{\mathrm{J}}$| . | |$\mathcal {M}$| . | |$B_0\, (\mathrm{\mu G})$| . | |$\mathcal {M_{\mathrm{A}}}$| . | |$\mu _{\mathrm{B}}$| . | |$\beta$| . | |$N_{\mathrm{sims}}$| . | |$N_{\mathrm{tot}}$| . | |$\overline{M}_{\mathrm{median}}\, (\mathrm{M_\odot })$| . | |$\overline{M}_{\mathrm{average}}\, (\mathrm{M_\odot })$| . | |$\overline{M}_{50}\, (\mathrm{M_\odot })$| . |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . | (9) . | (10) . | (11) . | (12) . | (13) . | (14) . | (15) . |
| |$\alpha _{\mathrm{vir}}= 0.0625$| | 2 | |$5.25\times 10^{-20}$| | 6200 | 2091.0 | 5 | 10 | 2.9 | 19.7 | 0.7 | 1 | 517 | |$0.25\pm 0.02$| | |$0.50\pm 0.05$| | |$1.04\pm 0.19$| |
| |$\alpha _{\mathrm{vir}}= 0.125$| | 2 | |$2.62\times 10^{-20}$| | 3100 | 737.1 | 5 | 28 | 2.9 | 13.7 | 0.7 | 2 | 520 | |$0.27\pm 0.05$| | |$0.46\pm 0.08$| | |$0.93\pm 0.15$| |
| |$\alpha _{\mathrm{vir}}= 0.5$| | 2 | |$6.56\times 10^{-21}$| | 775 | 92.4 | 5 | 20 | 2.9 | 6.9 | 0.7 | 10 | 449 | |$0.46\pm 0.06$| | |$0.73\pm 0.08$| | |$1.38\pm 0.16$| |
Note. Column 1: MHD simulation models with different virial parameter |$\alpha _{\mathrm{vir}}$|. Column 2: size of the cloud/computational domain. Columns 3: initial mean gas density. Column 4: total mass of the cloud. Columns 5: number of Jeans masses in the cloud. Column 6: rms sonic Mach number. Column 7: initial magnetic field strength. Column 8: Alfv|$\acute{\text{e}}$|n Mach number. Column 9: mass-to-flux ratio. Column 10: plasma beta (thermal-to-magnetic pressure ratio). Column 11: number of simulations (random seeds for the turbulence driving) performed. Column 12: total number of sink particles formed. Column 13: median stellar mass. Column 14: mean stellar mass. Column 15: |$M_{\mathrm{50}}$|, which is the median mass in a cumulative mass function. Quantities in Columns (13)–(15) are averaged over the SFE range |$1-5~{{\ \rm per\ cent}}$| (represented by overbars).
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