Evolution of the median of the disk radius, the disk mass, the disk temperature, and the mass accretion rate onto the primary as a function of the SFE for the NO_OUTFLOWS (blue) and OUTFLOWS (orange) models. The regions with transparent colors represent the area between the first and third quartile of the distribution. One can clearly see that outflows do not significantly impact the disk size and mass but largely influence their temperature through a reduced accretion rate (and luminosity).