Influence of the DR on the power injected in the acoustic mode (n = 7, ℓ = 0, m = 0) in a 1  M_⊙, Z = 0.02 solar-like model. Anti-solar regimes, characterised by $\mathrm{\Delta }\mathrm{\Omega }/\stackrel{\sim }{\mathrm{\Omega }}<0$, are represented in red, whereas solar DR regimes are shown in blue. The uniform rotation regime is indicated with a thicker dashed black line. For $\stackrel{\sim }{\mathrm{\Omega }}>1{\mathrm{\Omega }}_{\odot }$, such a solar-like star is unlikely to present an anti-solar DR because ℛo_f < 1. Thus, we represent this regime with dashed lines.