Fig. 5
Donor light contribution with respect to the total light calculated from the light curve model. Each curve shows the donor contribution for a specific spectral range around a spectral line. The selected spectral lines (and ranges) are from top to the bottom: HeI 6678 Å, Hα, HeI 5875 Å, Hβ, HeI 4471 Å, and Hγ. L1 and L2 are the stellar fluxes and Ld is the disc contribution.
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