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We take the recently published data of twin kHz quasi-period oscillations (QPOs) in neutron star (NS) lowmass X-ray binaries (LMXBs) as the samples, and investigate the morphology of the samples, which focuses on the quality factor, peak…

High Energy Astrophysical Phenomena · Physics 2015-03-17 J. Wang , H. K. Chang , C. M. Zhang , D. H. Wang , L. Chen , J. L. Qu , L. M. Song

We analyzed the recently published kHz QPO data in the neutron star low-mass X-ray binaries (LMXBs), in order to investigate the different correlations of the twin peak kilohertz quasi-eriodic oscillations (kHz QPOs) in bright Z sources and…

Astrophysics · Physics 2009-11-11 C. M. Zhang , H. X. Yin , Y. H. Zhao , F. Zhang , L. M. Song

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 (\nu) distribution of twin kHz QPOs…

High Energy Astrophysical Phenomena · Physics 2014-04-25 D. H. Wang , L. Chen , C. M. Zhang , Y. J. Lei , J. L. Qu

A recently published study on long term evolution of the frequencies of the kilohertz quasi-periodic oscillations (QPOs) in the atoll source 4U 1636-53 concluded that there is no preferred frequency ratio in a distribution of twin QPOs that…

We study in a systematic way the quality factor of the lower and upper kHz QPOs in a sample of low luminosity neutron star X-ray binaries, showing both QPOs varying over a wide frequency range. The sample includes 4U 1636-536, 4U 1608-522,…

Astrophysics · Physics 2009-11-11 Didier Barret , Jean-Francois Olive , M. Coleman Miller

We investigate the quality factor and RMS amplitude of the lower kHz QPOs from XTE J1701-462, a unique X-ray source which was observed in both the so-called Z and atoll states. Correcting for the frequency drift of the QPO, we show that, as…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Didier Barret , Matteo Bachetti , M. Coleman Miller

We report the discovery ($20\sigma$) of kilohertz quasi-periodic oscillations (kHz QPOs) at ~ 690 Hz from the transient neutron star low-mass X-ray binary EXO 1745-248. We find that this is a lower kHz QPO, and systematically study the time…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Arunava Mukherjee , Sudip Bhattacharyya

{We investigate the coherence of the twin kilohertz quasi-periodic oscillations (kHz QPOs) in the low-mass X-ray binary (LMXB) theoretically. The profile of upper kHz QPO, interpreted as Keplerian frequency, is ascribed to the radial extent…

High Energy Astrophysical Phenomena · Physics 2015-05-20 J. Wang , C. M. Zhang , Y. H. Zhao , Y. F. Lin , H. X. Yin , L. M. Song

We analyzed all published frequencies, nu_1 and nu_2, of the twin kilohertz quasi-periodic oscillations (kHz QPOs) in bright neutron star low-mass X-ray binaries. The two frequencies are well correlated but, contrary to recent suggestions,…

Astrophysics · Physics 2009-11-10 Tomaso Belloni , Mariano Mendez , Jeroen Homan

The kilohertz quasi-periodic oscillations (kHz QPOs) have been found in neutron star low mass X-ray binaries (NS-LMXBs), which present the millisecond timing phenomena close to the surface of the compact objects. We briefly summarize the…

High Energy Astrophysical Phenomena · Physics 2013-05-14 Chengmin Zhang , Dehua Wang

The width (W), root mean squared amplitude (Rs) of lower and upper kHz quasi-periodic oscillations (QPOs) from accreting neutron stars vary with frequency. Similarly, the QPO frequency varies with the source count rate (S). Hence, the…

High Energy Astrophysical Phenomena · Physics 2015-05-14 Martin Boutelier , Didier Barret , Yongfeng Lin , Gabriel Torok

AIMS: For six neutron-star atoll sources (4U 1608-52, 4U 1636-53, 4U 0614+09, 4U 1728-34, 4U 1820-30 and 4U 1735-44) we investigate the relationship between the observed fractional rms amplitudes of the twin kHz QPOs. We discuss whether…

Astrophysics · Physics 2010-11-02 Gabriel Torok

The recently updated data of the twin kilohertz quasi-periodic oscillations (kHz QPOs) in the neutron star low-mass X-ray binaries are analyzed. The power-law fitting $\nu_{1}=a(\nu_{2}/1000)^{b}$ and linear fitting $\nu_{2}=A\nu_{1}+B$ are…

Astrophysics · Physics 2009-06-23 H. X. Yin , Y. H. Zhao

We infer the emission positions of twin kilohertz quasi-periodic oscillations (kHz QPOs) in neutron star low mass X-ray binaries (NS-LMXBs) based on the Alfven wave oscillation model (AWOM). For most sources, the emission radii of kHz QPOs…

High Energy Astrophysical Phenomena · Physics 2015-10-07 D. H. Wang , L. Chen , C. M. Zhang , Y. J. Lei , J. L. Qu , L. M. Song

We report on a detailed analysis of the so-called ~1 Hz quasi-periodic oscillation (QPO) in the eclipsing and dipping neutron-star low-mass X-ray binary EXO 0748-676. This type of QPO has previously been shown to have a geometric origin.…

High Energy Astrophysical Phenomena · Physics 2015-11-13 Jeroen Homan , Joel K. Fridriksson , Ronald A. Remillard

We study the dependence of kHz quasi-periodic oscillation (QPO) frequency on accretion-related parameters in the ensemble of neutron star low-mass X-ray binaries. Based on the mass accretion rate, $\dot{M}$, and the magnetic field strength,…

High Energy Astrophysical Phenomena · Physics 2016-11-23 M. Hakan Erkut , Şivan Duran , Önder Çatmabacak , Onur Çatmabacak

We re-examine the correlation between the frequencies of upper and lower kHz quasi-periodic oscillations (QPO) in bright neutron-star low-mass X-ray binaries. By including the kHz QPO frequencies of the X-ray binary Cir X-1 and two…

Astrophysics · Physics 2008-11-26 T. Belloni , M. Mendez , J. Homan

We studied the correlations between spin frequencies and kilohertz quasi-periodic oscillations (kHz QPOs) in neutron star low mass X-ray binaries. The updated data of kHz QPOs and spin frequencies are statistically analyzed. We found that…

Astrophysics · Physics 2007-08-28 H. X. Yin , C. M. Zhang , Y. H. Zhao , Y. J. Lei , J. L. Qu , L. M. Song , F. Zhang

Double peak kHz QPO frequencies in neutron star sources varies in time by a factor of hundreds Hz while in microquasar sources the frequencies are fixed and located at the line \nu_2 = 1.5 \nu_1 in the frequency-frequency plot. The crucial…

Astrophysics · Physics 2007-05-23 M. A. Abramowicz , D. Barret , M. Bursa , J. Horak , W. Kluzniak , P. Rebusco , G. Torok

Using archival data from the Rossi X-ray Timing Explorer (RXTE), we study in a systematic way the variation of the quality factor and amplitude of the lower and upper kHz quasi-periodic oscillations (QPO) in the low-mass X-ray binary…

Astrophysics · Physics 2016-08-30 Didier Barret , Jean-Francois Olive , M. Coleman Miller
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