GOLUCHOVÁ, Kateřina, Andrea KOTRLOVÁ, Zdeněk STUCHLÍK and Gabriel TÖRÖK. Test of the Resonant Switch Model by Fitting the Data of Twin-Peak HF QPOs in the Atoll Source 4U 1636?53. Acta Astronomica. PL - Polská republika, 2014, vol. 64, No 1, p. 45-64. ISSN 0001-5237.
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Basic information
Original name Test of the Resonant Switch Model by Fitting the Data of Twin-Peak HF QPOs in the Atoll Source 4U 1636?53
Authors GOLUCHOVÁ, Kateřina, Andrea KOTRLOVÁ, Zdeněk STUCHLÍK and Gabriel TÖRÖK.
Edition Acta Astronomica, PL - Polská republika, 2014, 0001-5237.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Confidentiality degree is not subject to a state or trade secret
WWW URL
Organization unit Faculty of Philosophy and Science in Opava
UT WoS 000335538700004
Keywords in English accretion, accretion disks; stars: neutron; X-rays: binaries
Tags EE2-3-20-0071, , GB14-37086G
Tags International impact, Reviewed
Links EE2.3.20.0071, research and development project. GB14-37086G, research and development project.
Changed by Changed by: Jan Vlha, učo 48995. Changed: 27/4/2021 09:43.
Abstract
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 regionsrelated 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
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