Fig. 2

Normalised amplitudes, , as a
function of the inclination. The continuous line represents the ℓ1,k-16,m-1
unstable mode of the 2.9 M⊙ model. Dashed and dot-dashed
lines show the ℓ1,k-16,m-1
and ℓ1,k-12,m0
unstable modes of the 3.2 M⊙ model, respectively. Both models
are ~20 Myr old. Black,
blue, and red colours correspond to rotations of 0.20, 0.40, and 0.60 Ωcrit, respectively. The
largest amplitudes, maxAp(θ),
reached by each mode are used for the normalisation.
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