All Tables

Table 1: The first eight largest eigenvalues $\sigma$ for the free wave solutions of Eq. (43). Values are normalized to the frequency of the ISCO, $\Omega _{\rm isco}=6^{-3/2}$ . Results are given for 3 azimuthal modes m=1,2,5 for the Newtonian, as well as for the Schwarzschild gravitational field. Where no inner Lindblad resonance exist, this is represented by -.
Table 2: Value of the orbital frequencies at the parametric resonance radii for the first five orders n in the case of a Newtonian gravitational potential. The results are given for a $1.4~{M_\odot}$ neutron star rotating at 300 and $600~{\rm Hz}$ respectively. The value to the left of the symbol / corresponds to the absolute value sign taken to be - and on the right to be +. The -- sign indicates that no resonance condition can be satisfied.
Table 3: Value of the orbital frequencies at the parametric resonance radii for the first five orders n in the general relativistic case. The results are given for a $1.4~{M_\odot}$ neutron star rotating at 300 and $600~{\rm Hz}$ respectively. The value to the left of the symbol / corresponds to the absolute value sign taken to be - and on the right to be +.