Fig. 3.
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5063−5257 Å (top) and 5608−5869 Å (bottom) regions of uncorrected disentangled spectra of the primary and the secondary components of LX Mus with selected spectral lines identified. The red lines denote the atmosphere model fits to the observed spectra (blue). The grey-shaded areas were excluded from calculations by the use of an individual mask.
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