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Fig. 6.

image

Variation rate of the core angular velocity Ωc as a function of gravity for rotating models of the six subgiants. These models are computed without an additional transport of angular momentum (νadd = 0). Magenta, red, black, blue, green and cyan lines correspond to stars A, B, C, D, E and F, respectively. Vertical dashed lines indicate the values of the gravity for the six stars. A zoom during the subgiant phase is shown in the insert.

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