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Fig. 10.
Predicted emergent flux profiles for the rotating star models with Ω = [0, 0.5, 0.7, 0.9] (see Table 3). Upper and lower panels: intermediate and strong line with kL = 103 and kL = 105, respectively. The inclination angle has been set to sin(i) = [0, 0.707, 1] from left to right.
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