About: Test of the Resonant Switch Model by Fitting the Data of Twin-Peak HF QPOs in the Atoll Source 4U 1636–53     Goto   Sponge   Distinct   Permalink

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Description
  • Resonant Switch (RS) model has recently been proposed as an alternative to the standard models of twin-peak high-frequency quasi-periodic oscillations (HF QPOs) observed in low-mass X-ray binaries containing a neutron star. The model assumes switch of twin oscillations at a resonant point, where frequencies of the upper and lower oscillations \nu_U and \nu_L become commensurable and one pair of the oscillating modes (corresponding to a specific model of HF QPOs) changes to some other pair due to non-linear resonant phenomena. We test the RS model for the atoll source 4U 1636–53, where we assume two resonant points observed at frequency ratios \nu_U : \nu_L = 3 : 2, 5 : 4, by fitting the pairs of the oscillatory modes to the observed data in the regions related to the resonant points. Among acceptable variants of the RS model the most promising are those combining the relativistic precession (RP) and the total precession (TP) frequency relations or their modifications. The precision of the fits is shown to be strongly increased in comparison to fits realized by individual pairs along the whole data range. We demonstrate that the \chi^2 test is significantly improved. Fitting of the HF QPO data in the source 4U 1636–53 by the RP1–RP variant of the RS model gives the best results and implies that the neutron star mass and dimensionless spin are M \approx 2.2 M_{Sun} and a \approx 0.27.
  • Resonant Switch (RS) model has recently been proposed as an alternative to the standard models of twin-peak high-frequency quasi-periodic oscillations (HF QPOs) observed in low-mass X-ray binaries containing a neutron star. The model assumes switch of twin oscillations at a resonant point, where frequencies of the upper and lower oscillations \nu_U and \nu_L become commensurable and one pair of the oscillating modes (corresponding to a specific model of HF QPOs) changes to some other pair due to non-linear resonant phenomena. We test the RS model for the atoll source 4U 1636–53, where we assume two resonant points observed at frequency ratios \nu_U : \nu_L = 3 : 2, 5 : 4, by fitting the pairs of the oscillatory modes to the observed data in the regions related to the resonant points. Among acceptable variants of the RS model the most promising are those combining the relativistic precession (RP) and the total precession (TP) frequency relations or their modifications. The precision of the fits is shown to be strongly increased in comparison to fits realized by individual pairs along the whole data range. We demonstrate that the \chi^2 test is significantly improved. Fitting of the HF QPO data in the source 4U 1636–53 by the RP1–RP variant of the RS model gives the best results and implies that the neutron star mass and dimensionless spin are M \approx 2.2 M_{Sun} and a \approx 0.27. (en)
Title
  • Test of the Resonant Switch Model by Fitting the Data of Twin-Peak HF QPOs in the Atoll Source 4U 1636–53
  • Test of the Resonant Switch Model by Fitting the Data of Twin-Peak HF QPOs in the Atoll Source 4U 1636–53 (en)
skos:prefLabel
  • Test of the Resonant Switch Model by Fitting the Data of Twin-Peak HF QPOs in the Atoll Source 4U 1636–53
  • Test of the Resonant Switch Model by Fitting the Data of Twin-Peak HF QPOs in the Atoll Source 4U 1636–53 (en)
skos:notation
  • RIV/47813059:19240/14:#0005067!RIV15-MSM-19240___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • I, P(EE2.3.20.0071), P(GB14-37086G), S
http://linked.open...iv/cisloPeriodika
  • 1
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 50026
http://linked.open...ai/riv/idVysledku
  • RIV/47813059:19240/14:#0005067
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • accretion, accretion disks; stars: neutron; X-rays: binaries (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • PL - Polská republika
http://linked.open...ontrolniKodProRIV
  • [865398D55C6C]
http://linked.open...i/riv/nazevZdroje
  • Acta Astronomica
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 64
http://linked.open...iv/tvurceVysledku
  • Kotrlová, Andrea
  • Stuchlík, Zdeněk
  • Török, Gabriel
  • Goluchová, Kateřina
http://linked.open...ain/vavai/riv/wos
  • 000335538700004
issn
  • 0001-5237
number of pages
http://localhost/t...ganizacniJednotka
  • 19240
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