Fig. 3.
Spectral fit for MBO1. Upper panel: spectral energy distribution with photometry from UV, optical, and infrared bands (blue boxes) fitted to the model SED (red solid line). Lower panels: normalized VLT-FLAMES spectra (blue solid line), overplotted with the PoWR model (red dashed line). The atmospheric parameters and abundances of this best-fit model are given in Tables 3 and 4.
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