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Fig. 6

image

Comparison of the period-spacing pattern of 43 Cyg with a selection of period-spacing patterns detected for γ Dor stars observed with the Kepler space mission. The non-uniform variations of the period-spacings of 43 Cyg, caused by chemical gradients in the stellar interior, are clearly visible. The tilt in the pattern, caused by the stellar rotation, follows the trend established by the other observations.

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