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Fig. 5


Comparison of the observed spectra (blue histogram), the magnetic synthetic spectra, yielding the best fit to the observations (black thick line) and the non-magnetic synthetic spectra (grey thin line) for the three lines of interest Fe i 15 622 Å (left), Fe i 15 648.5 Å (middle), and Fe i 15 662 Å (right) of CHXR 28.

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