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Fig. B.5.
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Comparison of CTIO/CHIRON observed spectra (one per night) with synthetic spectra, for the model with χ2 = 3639180. The fit is acceptable, including the Hα, Hβ wings, with a notable exception of the Hα, Hβ core depths for Aa, Ab components (see red circles for spectra with higher signal-to-noise ratio).
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