Super-Spinning Compact Objects and Rapid Variability of Galactic Microquasars

In our previous work we applied several models of high-frequency quasi-periodic oscillations to estimate the spin of the central compact object in three Galactic microquasars. We also assumed the possibility that the central compact body is a super-spinning object. Here we extend our consideration and investigate in a consistent way the implications of several resonance models so far discussed only in the context of black holes.