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Fig. 2.
Equatorial and polar radius as a function of the fractional abundance of hydrogen in the convective core for a 5 M⊙ star initially rotating at ωi = 0.5 for Z = 0.02 and Z = 10−3. The stellar radius in case of no rotation has been added for comparison in full and dashed black lines for Z = 0.02 and 10−3 respectively.
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