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Fig. 5.
MS B-type stars showing coherent g mode pulsations. Light curves (left) and their corresponding LS-periodograms (right) for HD 57539, HD 35912, HD 41753, HD 48977, HD 26912 and HD 37711. No significant variability is seen beyond 4 d−1. The markers in the LS-periodograms have the same meaning as in Fig. 4.
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