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Fig. 6
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UV spectra of burst models for ages between 1 and 2.5 Myr. Coloured lines are models including VMSs, black lines models without VMSs (i.e. BPASS models). The dark (light) colours correspond to mass-loss rates not scaled (scaled) with metallicity. The left (middle, right) panel is for Z = 0.2 (0.1, 0.01) Z⊙.
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