  We investigate dynamical effects of particles moving around rotating SV
regular BH and traversable wormholes, and the deviation from Kerr BH. We found
that the rotating SV traversable wormhole spacetime has a closer innermost
stable circular orbit to the central object than Kerr and rotating regular BHs.
Furthermore, the paper provides the general form of the epicycle frequency in
this spacetime, presenting the radial profile of the angular frequency of
particles undergoing oscillatory motion. Unlike the commonly used $\chi$-square
analysis method, with considering a generalized data analysis approach in this
paper we hypothesize that the observational data of three microguasars can be
explained through an axisymmetric SV spacetime, fitting the data to find the
range of spin values for three types of SV objects, and analyzing the possible
mechanisms of HFQPOs (high-frequency quasi-periodic oscillations) generation
for different types of axisymmetric SV objects. We found that for a Kerr BH
with $l^*=0$, the observational data of three microquasars can be explained by
the HFQPOs model used in this paper (excluding ER4 model); for a regular BH
with $l^*=1$, the HFQPO phenomenon observed through the three microquasars can
be explained by the ER0, ER1, ER2, ER3, RP0, RP1, RP2, TD and WD models. For a
traversable wormhole with $l^*=3$, the mechanism of HFQPO can be interpreted by
the ER1, ER3, RP0, RP1, RP2, TD and WD models. Moreover, we observed that for
the same HFQPOs model, the limiting range of the spin parameter $\alpha^*$
increases with the increase of the parameter $l^*$.
