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Fig. 7.

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Generalised Hough functions (normalised) as a function of the horizontal coordinate x at different pseudo-radii from ζ = 0.153 (blue) to ζ = 1 (yellow) at Ω/ΩK = 0.2 for gravity-like solutions {k = 0, m = 1} with ωin = 10−4 rad s−1 corresponding to (the solid lines) and Rossby-like solutions {k = −2, m = −1} with ωin = −5.5 × 10−5 rad s−1 corresponding to (the dotted lines) in the case of a star: (a) uniformly rotating, (b) differentially rotating according to the pseudo-radius, (c) differentially rotating according to the colatitude and (d) differentially rotating according to the pseudo-radius and the colatitude.

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