Stellar companions and Jupiter-like planets in young associations

Open Access

Fig. 20

Run of the mass accreted from the interstellar matter to the disk with the episode of accretion for the best-fit parameters of the toy model for the formation of binaries by disk instability appropriate for early-B (M_A = 7.25 M_⊙), late-B (M_A = 2.43 M_⊙), and solar-type stars (M_A = 1.04 M_⊙).

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