Table 1:
Upper half: The four a priori possible types of dynamical states of accretion structures, corresponding to the division of the dynamical parameter space into fast-slow rotation and large-small pressure. Lower half: A different division of the parameter space, corresponding to high-low accretion rate and large-small opacity. |
Table 2:
Frequency ratio of the “twin peak” QPOs in all four microquasars where they have been detected. |
http://www.livingreviews.org/lrr-2013-1 |
Living Rev. Relativity 16, (2013), 1
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