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Fig. 5
Effect of fast rotation on the surface shape of CU Vir. The stellar shape is shown here for Teff = 12 750 K, M = 3.06 M⊙, Prot = 0.5207130 d and different combinations of i and vesini adopted in the Doppler imaging studies of this star. The stellar rotational axis corresponds to a line at x = 0.
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