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Fig. 4.

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Example of fits to N lines for our target stars. In this case, the N II 3995 Å line is shown for V1034 Sco (primary star on the left, secondary star on the right). The blue lines show the re-normalised disentangled spectra of the stars. The red lines show synthetic spectra from our pre-calculated grid for three different abundances (labelled in the bottom-right corner in each panel).

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