New predictions for radiation-driven, steady-state mass-loss and wind-momentum from hot, massive stars - II. A grid of O-type stars in the Galaxy and the Magellanic Clouds

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Fig. 8

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Value of the exponent n showing the metallicity dependence of D_mom together with a linear fit, showing the linear dependence of this exponent with log (L_* ∕10⁶ L_⊙). See text for details.

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