...)[*]
Interestingly, the same 3:2 ratio seems to be present in the case of neutron stars sources, indicating the same origin of the observed quasiperiodic oscillations (Abramowicz et al. 2003; see however, Belloni et al. 2004).
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...$a\in (-1,~1)$[*]
Here and henceforth values of a > 0 correspond to corotating orbits, while a < 0 give counterrotating orbits.
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... derivatives[*]
After introducing $^\prime$ as ${\rm d}/{\rm d}r$.
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... maxima[*]
We distinguish which is the global one in Sect. 4.
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... with[*]
Here and henceforth in relation to the wave propagation in the field of black holes $\omega_{{\rm max}}$ denotes the maximum of $\omega _{\rm r}$ at $\mathcal{R}_{\rm r}(a)$ (Fig. 2) in the black-hole range of the rotational parameter.
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... with[*]
In the relation to the wave propagation in discs around Kerr naked singularities, $\omega_{~{\rm MAX}}$ denotes the global maximum of $\omega _{\rm r}$, while $\omega_{{\rm max}}$ denotes a local (lower) one, see Fig. 8.
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... [*]
Intuitively clear attribution is well founded in the last Sect. 4.4.
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... when[*]
We note that the same condition holds for internal resonance, which describes systems with conserved energy (Horák et al. 2004).
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... disc[*]
Such a claim is motivated by experience from known situations related to the parametric or forced resonance in complex non-linear systems observed in Earth physics (Landau & Lifshitz 1976). Examples of mathematically possible resonances causing damaging bridges, wings, etc. with no specific physical coupling mechanism known are discussed in Nayfeh & Mook (1979).
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Copyright ESO 2005