Fig. 8.
Variability of the spectrum near the Hα emission line of the intermediate accretor 06401111+0921272 (upper panel) and of the class II accretor 06404136+0954138 (lower panel) for all the 20 original spectra collected for each of these stars. We note that to avoid confusion, the spectra are not continuum-normalized and, thus, the continua are different.
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