Seismic diagnostics for transport of angular momentum in stars - I. Rotational splittings from the pre-main sequence to the red-giant branch

J. P. Marques; M. J. Goupil; Y. Lebreton; S. Talon; A. Palacios; K. Belkacem; R.-M. Ouazzani; B. Mosser; A. Moya; P. Morel; B. Pichon; S. Mathis; J.-P. Zahn; S. Turck-Chièze; P. A. P. Nghiem

doi:10.1051/0004-6361/201220211

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Volume 549 (January 2013)

A&A, 549 (2013) A74

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Fig. 13

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Top: rotational splittings δν_nℓ for ℓ = 1 modes as a function of the normalized frequency ν/Δν associated with the rotation profile shown in Fig. 12 for the 1.2 M_⊙ model. Middle: corresponding δν/β_nℓ for ℓ = 1 modes as a function of the normalized frequency ν/Δν. Bottom: the same for ℓ = 2 modes.

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