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. 4

$Δ \log \dot{M}$ $Mathematical equation: $\Delta \log \dot M$$ vs T_eff. $\dot{M}$ $Mathematical equation: ${\dot M}$$ is the difference between our derived ∆ log M˙ and those obtained from numerical recipes from Vink & Sander (2021) (yellow dots), Björklund et al. (2023) (blue dots), and Krtička et al. (2024) (red dots).

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