Fig. 6.

Correlation between observed frequency νQPO and the Kepler frequency at the transition radius νK(rJ) (top), as well as the residuals defined as the ratio between the best weighted fit (in red) and the data (bottom). In their own colors, different types of quasi-periodic oscillations: Type A in light-yellow, Type B in cyan, Type C in dark-blue. In red the weighed linear fit considering only Type C LFQPOs, νQPO = (10 ± 3) × 10−3 ⋅ νK(rJ)0.96 ± 0.04, in black the νQPO = νK(rJ)/100 line.
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