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Fig. B.3
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Normalised far-UV HST-STIS/G140L, optical HST-STIS/G430M, Hα G750M and K-band VLT/SINFONI observations (blue line), which is compared to the synthetic composite spectra from our best-fit fixed-M R136a1 model with vturb = 100 km s−1 (red line).
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