Fig. 5.
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Angular velocity as a function of mass coordinate at different moments during the first helium flash of the 1.5 M⊙ model presented in Fig. 4. Radiative regions are shown as solid lines, while convective regions are shown as dotted lines. The inset around Mr/M ∼ 0.32 shows a zoomed-in image of the location of the H-burning shell.
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