Fig. 17
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Comparison between burst population synthesis models including VMSs up to 225 M⊙ and the observed UV spectrum of MrK71-A (black line). Top (bottom) models are for Z = 0.2 (0.1) Z⊙. In each panel ages range from 0 to 2.5 Myr from top to bottom. The left (right) panels correspond to models without (with) metallicity scaling of the VMS mass-loss rates.
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