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Fig. 5

image

Top: part of the Fourier spectrum where the period-spacing pattern was found, with the pulsation periods of the pattern marked by dashed lines. Middle: detected period-spacing pattern. Bottom: two model period-spacing patterns, for M = 1.6 M, solar metallicity, αMLT = 1.8, fov = 0.015 Hp, and Xc = 0.36. The models have a constant extra diffusive mixing Dmix in the radiative region of 0 cm2 s-1 (full black) and 1 cm2 s-1 (dashed grey), respectively.

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