Fig. A.1
Mass spectra of runs A0, A1d, A2, and A2d, with the same color coding as in Fig. 6. The cloud with a radius of 0.75 pc is evolved without gravity on levels 8 or 9 during 0, 0.3, and 0.6 turbulence-crossing times. With longer relaxation, more massive stars develop, and the IMF is slightly more top-heavy.
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