Magnetic fields or overstable convective modes in HR 7495 - Exploring the underlying causes of the spike in the ‘hump and spike’ features

Open Access

Fig. 10.

Upper panel: Amplitudes determined for subsets of the Kepler data spanning 150 days. The BJD corresponds to the average value for each data bin. Uncertainties are smaller than the symbols depicted. Lower Panel: Phase differences. The average difference has been removed to enhance readability.

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