Figure 9.
Korel radial velocities from Hβ lines and TESS light curve of V881 Sco, and WD + MC model fitting. The solid red lines include proximity effects, whereas the dashed black lines correspond to Keplerian orbits for the RV models. Residuals to the LC model are plotted in the bottom figure.

Korel radial velocities from Hβ lines and TESS light curve of V881 Sco, and WD + MC model fitting. The solid red lines include proximity effects, whereas the dashed black lines correspond to Keplerian orbits for the RV models. Residuals to the LC model are plotted in the bottom figure.

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