Fig. D.1.
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Time evolution of the radiative flux Frad (top) and accretion energy flux Facc (bottom) since protostellar birth. Both panels show outcomes from a 1D spherical setup with different initial molecular cloud core masses using the PLUTO code. Also shown as black circles in both panels is data from a 3D RAMSES simulation with an initial turbulent Mach number of 0.2.
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