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Fig. 5.
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Geometries of the dominant (k, m) = (0, 1) g mode (left) and (k, m) = (−2, −1) r mode of KIC 3341457 (right), ignoring the effects of tidal deformation and perturbation. Regions on the stellar surface where the pulsations cause the temperature to decrease (increase), are indicated in red (blue).
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