Table 3
Spin functions a(xp:q) determined for the epicyclic forced resonance QPO models.
Model | Spin function | a p:q |
![]() |
||
|
||
Ep1 |
![]() |
1.08471 |
1.00119 | ||
|
||
Ep2 |
![]() |
1.07331 |
1.01193 | ||
|
||
Ep3 |
![]() |
1.08807 |
1.00006 | ||
|
||
Ep4 |
![]() |
1.08123 |
1.00337 | ||
|
||
Ep5 |
![]() |
1.06226 |
1.03363 |
Notes. There are two separate branches of solution for each model, the “−” sign applies to black holes and naked singularities with 1 <a ≲ ap:q, while the “+” sign applies to naked singularities with a ≳ ap:q. The last column indicates the value of ap:q for each model as well as the related spin value , where the a(xp:q) function has a local maximum, which implies the “S-like” behaviour of resonant radii xp:q(a) and the existence of three resonant radii for
(see Fig. 3b).
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