From core to envelope: Revealing the deep dynamics of stars with two convective zones

Open Access

Fig. 9.

Six-day chunk of the time series obtained for v_obs after filtering, at r/R_★ = 0.97 (top row), averaged in the convective envelope (0.88 ≤ r/R_★ ≤ 0.97, middle row), and r/R_★ = 0.80 (bottom row), for the Full (left column) and the EnvCZ (right column) models, respectively.

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