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Fig. 8

image

Spectral energy distribution fit of a sample B star (N206-FS 147). The model SED (red) is fitted to the available photometry from optical (UBV RI), near-infrared (JHKs), and mid-infrared (IRAC 3.6, 4.5, and 8.0 μm) bands (blue boxes) as well as the flux calibrated UV spectra from the HST. The luminosity L and the color excess EBV of the best-fitting model are given in the figure.

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