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arXiv · 1301.5478

Statistical properties of twin kHz QPO in neutron star LMXBs

D. H. Wang·L. Chen·C. M. Zhang·Y. J. Lei·J. L. Qu
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Abstract

We collect the data of twin kilohertz quasi-periodic oscillations (kHz QPOs) published before 2012 from 26 neutron star (NS) low-mass X-ray binary (LMXB) sources, then we analyze the centroid frequency (ν) distribution of twin kHz QPOs (lower frequency ν_1 and upper frequency ν_2) both for Atoll and Z sources. For the data without shift-and-add, we find that Atoll and Z sources show the different distributions of ν_1, ν_2 and ν_2/ν_1, but the same distribution of Δν(difference of twin kHz QPOs), which indicates that twin kHz QPOs may share the common properties of LXMBs and have the same physical origins. The distribution of Δνis quite different from constant value, so is ν_2/ν_1 from constant ratio. The weighted mean values and maxima of ν_1 and ν_2 in Atoll sources are slightly higher than those in Z sources. We also find that shift-and-add technique can reconstruct the distribution of ν_1 and Δν. The K-S test results of ν_1 and Δνbetween Atoll and Z sources from data with shift-and-add are quite different from those without it, and we think that this may be caused by the selection biases of the sample. We also study the properties of the quality factor (Q) and the root-mean-squared (rms) amplitude of 4U 0614+09 with the data from the two observational methods, but the errors are too big to make a robust conclusion. The NS spin frequency (ν_s) distribution of 28 NS-LMXBs show a bigger mean value (about 408Hz) than that (about 281 Hz) of the radio binary millisecond pulsars (MSPs), which may be due to the lack of the spin detections from Z sources (systematically lower than 281 Hz). Furthermore, on the relations between the kHz QPOs and NS spin frequency ν_s, we find the approximate correlations of the mean values of Δνwith NS spin and its half, respectively.

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D. H. Wang, L. Chen, C. M. Zhang, Y. J. Lei, J. L. Qu. 2013-10-21. Statistical properties of twin kHz QPO in neutron star LMXBs. https://doi.org/10.1002/asna.201311995

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