Fig. 8
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Comparison between the [O I] 630 nm line profiles having Vp close to zero, and a model of emission from a Keplerian disk. In the observed profiles the NLVC (or the NLVC+BLVC in the cases of Type 2 profiles) has been isolated by subtracting the Gaussian fit derived for the other components at different velocities. The fitted parameters of the model are indicated in each panel.
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