Fig. 12
Doppler maps that combine the tomograms for different lines from the 2005 observations (left) and for the strongest lines from different sets of observations (right). The maps are zoomed around the emission region in the leading side of the accretion disc. The circular dashed lines represent Keplerian velocities at the tidal truncation (rmax) and 3:1 resonance (r3:1) radii.
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