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Fig. 1


Top: solid black line shows the profile of the Brunt-Väisälä frequency N0 normalised by ω0 for the non-rotating stellar model. The red lines show N0 for the Ω = 0.84ΩK model along the polar (solid line) and equatorial (dashed line) radii. A thick red tick on the x-axis indicates the polar radius Rp. Top: map in a meridional plane of N0 normalised by ω0 for the Ω = 0.84ΩK model. The black line is the star surface.

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