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Fig. 4

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Variation of mass-loss rate with metallicity for the scaled solar chemical composition. Upper panel: mean dependence of the ratio of the scaled solar chemical composition mass-loss rate on the solar metallicity mass-loss rate after Eq. (1). Middle panel: ratio of the mass-loss rate of individual model stars to the solar abundance mass-loss rate plotted relatively to the fit from the upper panel (Eq. (1)). Lower panel: variations of the steepness of the dependence of log [(Z) /(Z)] on log (Z/Z) (see Eq. (2)) with metallicity.

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