New line-driven wind mass-loss rates for OB stars with metallicities down to 0.01 Z⊙

Open Access

Fig. 2.

Power of the metallicity dependence of the mass-loss rate Ṁ ∼ Z^α (Eq. (1)) plotted as a function of the stellar effective temperature for models at different metallicities. Dashed lines describe mean relationship derived for individual metallicities.

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