Results of the core and the envelope rotation rates of our sample. The left column (panels a, b, c) shows the core rotation rates as a function of mixed mode density, stellar mass, and radius. The right column (panels d, e, f) is the counterpart of envelope rotations. The open points are the stars identified below the ΔΠ₁–Δν sequence in Fig. 14. The dashed lines in panel (a) circle the over-density ridge.