Fig. A.4.
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Total SFE (Mstar/Mcl) in six different GMCs. The clouds with weak and strong turbulence are plotted in the top and bottom panels, respectively. Different columns correspond to simulations with different random seeds for turbulence driving. Simulations with different resolutions are shown in different colors and line styles, as indicated in the legend. The star formation efficiency converges from runs with a resolution of ∼0.25 pc.
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