Notes. The table shows the model name, composed of the approximate effective temperature and surface gravity and of a running number; the mass M_⋆, used for the external potential; the envelope mass M_env, derived from integrating the mass density of all grid cells within the computational box; the average emitted luminosity L_⋆, close but not identical to the inserted luminosity of either 5000, 7000, or 10 000 L_⊙ in the core; the model dimensions n_x × n_y × n_z; the edge length of the cubical computational box x_box; the rotational period P_rot; the time t_avg, used for the averaging of the rest of the quantities in this table and for the further analysis; the average approximate stellar radius R_⋆; the average approximate effective temperature T_eff; the logarithm of the average approximate surface gravity log g; the pulsation period P_puls; and the half width of the distribution of the pulsation frequencies σ_puls. The first (“old”) group of simulations comprises models used in Freytag & Höfner (2008). In the second (“test”) group, numerical parameters (e.g., the box size or the number of grid points) or the rotation period were varied. The last (“grid”) group comprises models with slightly varying stellar parameters (M_env, L_⋆).