Fig. 1
Synthetic SEDs (in red) compared to flux calibrated + UBVJHK photometry for the target stars (in black). The distance, E(B − V) and luminosity were iterated to reach agreement between models and observations (see Sect. 4.1). For plotting purpose, the fluxes were scaled by a factor 1014 for all stars but HD 66811 and HD 210839, where factors 109 and 1013 were used, respectively.
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