Impact of wind variations on the density profiles of binary-stripped stars. We show the profiles at the moment of core helium depletion for a single (blue) and binary-stripped (red) star model with the same initial mass of 11 M_⊙ (top panel) and 20 M_⊙ (bottom panel). Gray lines show variations in the density profile for the binary-stripped star when we vary the wind mass-loss rate after Roche-lobe overflow by the factor indicated in the legend.