Angular momentum relaxation in models of rotating early-type stars

Open Access

Fig. 2.

Damping rate of the least-damped baroclinic mode in the spherical Boussinesq model as a function of the ratio N=N_*/2Ω_*, for $P = 0$ ${\mbox {${ {\cal {{P}}} }$}} = 0$ and E_t = 10⁻³. Dots represent numerical solutions, while the solid line corresponds to the approximate solution given by (14).

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