Fig. 24
Idem Fig. 22, but for star CoRoT 102686433 (star No 6) in the LRA1. The peak amplitude of each frequency group is variable through the light curve; transient frequenciesappear during the brightening phase (c) and form the broad groups at 1.15 and around 2.27 c d−1. This latter frequency appears double in the relaxation phase (d).
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