Fig. B.4.
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Upper limits for the near-core to envelope rotation rate deduced from Gaia DR3 measurements of vbroad available for 969, 965, and 929 gravity-mode pulsators in the sample of pulsators with a radius estimate from the Z = 0.014 (grey triangles), Z = 0.0080 (pink circles), and Z = 0.0045 (blue diamonds) model grids, respectively.
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