Radius evolution of low-metallicity stripped-star models with an initial mass of 10.5 M_⊙ as a function of time after core helium depletion. The blue curve represents a model computed with our default wind scheme, while the orange and green curves are for models with mass-loss rates 3 and 10 times higher than the default, respectively. The dashed red curve represents a low-metallicity model computed with the solar metallicity mass-loss scheme.