Temperature variations (blue = hot, red = cold) and displacements (white arrows) associated with a (k, m)=(0, 1) g mode at spin values of 0.58 (top) and 4.15 (bottom). These mode geometries match those of the (n, k, m)=(−30, 0, 1) pulsation evaluated in Fig. A.3 for a 1.5-M_⊙ stellar model with a core hydrogen fraction of X_c = 0.4, seen at an inclination angle of 60°, and rotating at 0.25 d⁻¹ (top) and 1.5 d⁻¹ (bottom), respectively.