Fig. 10
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Normalised far-UV HST-STIS/G140L, optical HST-STIS/G430M, Hα G750M observations from Crowther et al. (2016), and K-band VLT/SINFONI observations from Schnurr et al. (2009) in blue. They are compared to the normalised synthetic spectra from our best-fit fixed-clumping R136a1 model (red line). The far-UV HST data are normalised by dividing the absolute flux by the continuum of the model.
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