Top: ΔP vs P diagram for the $\stackrel{\sim }{\ell }=m=1$ modes in the 0.5 M_⊙ model in the co-rotating frame. The dots correspond to the modes computed considering the full extent of the stellar structure, with the slow case in orange, the intermediate case in yellow, and the fast case in blue. The vertical dashed lines mark the period of the modes computed considering only the convective envelope. The position of the Coriolis frequency, 2Ω, is highlighted for the slow, the intermediate, and the fast cases (vertical thick lines in orange, yellow, and blue, respectively), while the $\sqrt{2}\mathrm{\Omega }$ frequency is indicated with the vertical dotted lines. The location of the modes with the eigenfunctions represented in Fig. 3 is marked with the light blue stellar symbol. Bottom: Same as the top panel but for the 1 M_⊙ model.