Fig. 17.
Results of our simulations in the case where foverflow is amplified on 240 d. From top to bottom: variations in foverflow, the light curve for the V-band magnitude, and the disk radius in units of the binary separation. Here, foverflow is 0.5 after 240 d.

Results of our simulations in the case where foverflow is amplified on 240 d. From top to bottom: variations in foverflow, the light curve for the V-band magnitude, and the disk radius in units of the binary separation. Here, foverflow is 0.5 after 240 d.

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