All Tables

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).