Fig. 3
Spectral energy distribution of AzV 189, from FUV (COS spectrum) to NIR (data from Bonanos et al. 2010). The fit to the SED with a model with a luminosity derived with the procedure outlined in the text, to take into account the potential binarity of this system, is shown in red. We used a distance modulus DM = 18.9 and E(B − V)Gal = 0.037 and E(B − V)SMC = 0.1.
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