The role of magnetic fields in the formation of multiple massive stars

Open Access

Fig. 6.

Sums of all sink masses as a function of time. Left panel: sums of all sink masses in the HYDRO runs. The filled circles indicate the secondary formation epoch. Right panel: sums of all sink masses in the MU2 runs. In both panels, the blue region shows the value obtained in the highest resolution runs ±20%.

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