Fig. 2.
Region from 5229 to 5285 Å of uncorrected disentangled spectra of the primary (top) and the secondary (bottom) components of AL Ari, AL Dor, FM Leo and BN Scl with selected spectral lines identified. The red lines denote the atmosphere models fits to the observed spectra (blue). The rotational broadening of the absorption lines is easily visible in AL Ari and BN Scl.
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