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Fig. B.1.

Fig. B.1. Refer to the following caption and surrounding text.

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Top panel Growth rate σr normalised by Ω in the (Pm, Λϕ) plane of the axisymmetric AMRI, for a regime typical of DNS (see Table 1, with |Ro| = 0.05, ΛZ = 0, (N/Ω)2 = 1, m = 1). The three criteria (Eq. 9) correspond to the limits of the unstable parameter domain. The blank region corresponds to the stable parameter domain. Bottom panel Same study but for the stellar radiative regime set of parameters, |Ro| = 0.05, m = 1 and (N/Ω)2 = 10.

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