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. 2.

Original Kepler and TESS data (in grey) phase folded using the spike frequency derived from Kepler data. Coloured curves represent the binned data and show the median value in each of the 80 arbitrarily chosen bins.

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