Fig. 13
Section of the STIS observation around L α, compared with our final synthetic spectrum (thick, red, Teff = 70000 K, log g = 7.5). The dashed, blue lines are the pure photospheric model-atmosphere spectra (Teff = 70000 K, log g = 7.0,7.5,8.0), i.e., no interstellar line absorption is applied. See text for the description of inserts A and B.
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