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Fig. 2
Dependence of the predicted mass-loss rates for Z = Z⊙ (small blue crosses) in comparison with main sequence mass-loss rates of B stars (black line, Krtička 2014) and observed values for subdwarfs from Tables 2 and 3 (large red crosses). The star vZ 1128 is not plotted, since it is a Pop II star with different Z.
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