Fig. 3
Top panel: mode inertia versus mode frequencies for angular degrees ℓ = 0 and ℓ = 2. Mode inertias are computed by integrating the squared eigendisplacement over the stellar mass. Bottom panel: same as Fig. 2, except that 
is computed by considering the total contribution of the ℓ = 2 modes for the selected range displayed in red in the top panel.
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