Fig. 16
FWHα,10% values for the broad components from the Hα line decomposition, and EWs of Hα and Ca II λ3933 with respect to the orbital phases of GW Ori B. We divide the orbital phases into different bins and show the mean values in individual bins with filled squares, as well their standard deviations with error bars. The dashed line in each panel is the median value.
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