Fig. 4

Top: variation of the angular velocity
() as a
function of r during the computed evolution of the 1.1
M⊙ star
(Z = Z⊙). The colour scale used
allows the identification of the different fronts of extraction of the angular
momentum and their propagation speed. The shaded area indicates the convective
envelope, while the dotted white line corresponds to the limit of H-burning
(defined as ϵnuc ≤ 1 erg s-1).
Bottom: evolution of the loss of angular momentum during the
computed evolution of the 1.1 M⊙ star
(Z = Z⊙).
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