KOTRLOVÁ, Andrea, Zdeněk STUCHLÍK and Gabriel TÖRÖK. Resonant switch model of twin peak HF QPOs applied to the source 4U 1636-53. Acta Astronomica. PL - Polská republika, 2012, vol. 62, No 4, p. 389-407. ISSN 0001-5237.
Other formats:   BibTeX LaTeX RIS
Basic information
Original name Resonant switch model of twin peak HF QPOs applied to the source 4U 1636-53
Authors KOTRLOVÁ, Andrea, Zdeněk STUCHLÍK and Gabriel TÖRÖK.
Edition Acta Astronomica, PL - Polská republika, 2012, 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 000314616700005
Keywords in English Accretion; Accretion disks; Stars: neutron; X-rays: binaries
Tags , GA202-090772, GD205-09H033
Tags International impact, Reviewed
Links GA202/09/0772, research and development project. GD205/09/H033, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 7/4/2021 08:01.
Abstract
Resonant Switch (RS) model of twin peak high-frequency quasi-periodic oscillations (HF QPOs) assumes switch of twin oscillations at a resonant point where frequencies of the upper and lower oscillations VU and V L become commensurable and the twin oscillations change from one pair of the oscillating modes (corresponding to a specific model of HF QPOs) to some other pair due to nonlinear resonant phenomena. The RS model is used to determine range of allowed values of spin a and mass M of the neutron starlocated in the atoll source 4U 1636-53 where two resonant points are observed at frequency ratios VU: VL = 3:2,5:4. We consider the standard specific models of the twin oscillations based on the orbital and epicyclic geodetical frequencies. The resonantpoints are determined by the energy switch effect exhibited by the vanishing of the amplitude difference of the upper and lower oscillations. The predicted ranges of the neutron star parameters are strongly dependent on the twin modes ap
PrintDisplayed: 9/5/2024 01:21