Angular momentum relaxation in models of rotating early-type stars

Open Access

Fig. 5.

Variation of the least-damped eigenvalue associated with the least-damped baroclinic mode as a function of rotation rate Ω for the anelastic model with Γ₁ = 5/3, n = 3, E_t = 10⁻³, η = 0.18, Q = 1, and $P = 0$ ${ {\cal {{P}}}} = 0$ . The expected Ω²-dependence is shown as a dashed line.

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