Publication date: Aug 2017
Abstract:
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.
Authors:
Kotrlova, Andrea; Sramkova, Eva; Torok, Gabriel; Stuchlik, Zdenek; Goluchova, Katerina;