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Figure 3: Evidence for the existence of the ISCO from data recorded by the Rossi X-ray Timing
Explorer satellite from neutron star binary source 4U 1636–536 [33]. The source shows quasi-periodic
oscillations (QPOs) with frequencies in the range
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Figure 3: Evidence for the existence of the ISCO from data recorded by the Rossi X-ray Timing
Explorer satellite from neutron star binary source 4U 1636–536 [33]. The source shows quasi-periodic
oscillations (QPOs) with frequencies in the range
![]() ![]() |