Near-core rotation frequency f_rot versus asteroseismic gravity for two samples: 490 Kepler gravity- and gravito-inertial mode pulsators with prograde modes from Fritzewski et al. (2024a, orange circles) and 2447 gravito-inertial prograde dipole mode pulsators from Aerts et al. (2025a, blue crosses). The position of the same quantities for more than a thousand red giant stars from mixed-mode asteroseismology is indicated by the red rectangle produced from Aerts et al. (2019, Fig. 4).