Fig. 1.
1.7 M⊙ stellar model at Xc = 0.7 with frot,s = 2 d−1 and δ f = 0.0 (light grey), 0.1 (grey), and 0.2 (black). Top left: the Brunt-Väisälä frequency profile. Top right: the considered stellar rotation profiles. Left panels: the corresponding gravito-inertial mode pulsations with (k, m)=(+0, +1), computed from Eq. (3) (middle) and with GYRE v5.1 (bottom). Right panels: the corresponding gravito-inertial mode pulsations with (k, m)=(−2, −1), computed from Eq. (3) (middle) and with GYRE v5.1 (bottom).
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