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Fig. 2

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Comparison between δgeff and for three modes. The upper row shows the meridional cross-section of the three modes, whereas the lower row compares the two calculations for the perturbation to the effective gravity at the stellar surface, between one of the poles (θ = 0°) and the equator (θ = 90°). For the middle and right mode, the two curves nearly overlap, making it hard to distinguish them.

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