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Fig. 7.
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Angular velocity profiles versus the radius within the star for models 
(blue), 
(red), and 
(magenta) at [Fe/H] = +0.15 and for four masses: 1.0, 1.2, 1.3, and 1.4 M⊙ (the value of 
used is indicated for each mass). The solid, dashed, and dot-dashed lines refer to three different ages (0.6, 0.75, and 2 Gyrs, respectively).
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