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- W1657738706 abstract "Observations show that the upper νU and lower νL of the “twin peak” high frequency QPOs inneutron star sources vary along linesνU = AνL+B in a frequency-frequency plot, and that their ratios νU/νL cluster near the value 3/2. This behaviour is well consistent with the predictions of the non-linear resonance model for QPOs. In this Note, we further explore our recent finding that the coefficients A, B of the frequency-frequency lines for individual sources are anticorrelated. In the (A, B) plane, they occupy rather a narrow region along the line A = 3/2 − B/600 Hz. We show that this observational property of QPOs also follows from the resonance model." @default.
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- W1657738706 date "2005-12-01" @default.
- W1657738706 modified "2023-09-27" @default.
- W1657738706 title "A note on the slope-shift anticorrelation in the neutron star kHz QPOs data" @default.
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