X-Shooting ULLYSES: Massive stars at low metallicity - XIV. Properties of SMC late-O and B supergiants reveal the metallicity dependence of winds in the Magellanic Clouds

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Fig. 11

$\log {\dot{M}}_{t}$ $Mathematical equation: $\log {{\dot M}_{\rm{t}}}$$ versus T_eff. The solid blue line is a simple linear fit to the entire sample. The colour gradient correlates with the value of Γ_e.

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