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Fig. 10

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Characteristics of the broad line component: Top: flux amplitude; Middle: velocity shift of the line centre; Bottom: Gaussian width in km s-1. The legend applies to all panels. The earlier rise in the He i D3 line is caused by using a running mean for the fitting process. The high velocity shifts in Hα are caused by line subcomponents influencing the fit. The vertical bar in each panel represents a typical error bar.

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