Table 1: Sample parameters, name of the environment used in the text consisting of the Mach number  $\mathcal{M}$ and the driving scale k (GA denotes the model with Gaussian density), number  $\mathcal{N}$ of protostellar objects (i.e. "sink particles'' in the centers of protostellar cores) at the final stage of the simulation, percentage of accreted mass at the final stage $ M_{\rm acc}/M_{\rm tot}$, parameter  $\mathcal{A}$ see Eq. (5), parameter $\mathcal{B}$ see Eq. (9).
Name k $\mathcal{M}$ $\mathcal{N}$ $ M_{\rm acc}/M_{\rm tot}$ $\mathcal{A}$ $\mathcal{B}$
        $\left[\%\right]$ $\left[10^{20}\ {\rm cm^2~s^{-1}}\right]$
M2.0k2 1..2 2.0 68 75 1.7 1.7
M2.0k4 3..4 2.0 62 48 2.0 2.0
M2.0k8 7..8 2.0 11 66 1.7 1.6
M3.2k2 1..2 3.2 62 80 1.2 1.3
M3.2k4 3..4 3.2 37 82 2.0 1.9
M3.2k8 7..8 3.2 17 60 2.7 2.6
M6k2 1..2 6.0 110 76 1.3 1.3
M6k4 3..4 6.0 60 65 1.5 1.7
M6k8 7..8 6.0 7 4 1.9 1.4
M10k2 1..2 10.0 100 38 1.0 1.0
M10k4 3..4 10.0 10 6 2.0 1.4
M10k8 7..8 10.0 27 8 1.4 1.05
GA ... ... 56 85 1.4 1.05


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