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@inproceedings{42581,
author = {Kotrlová, Andrea and Stuchlík, Zdeněk and Török, Gabriel},
address = {Cambridge, UK},
booktitle = {Proceedings of the International Astronomical Union},
doi = {http://dx.doi.org/10.1017/S1743921312020194},
keywords = {Accretion; Accretion disks; Stars: neutron; X-rays: binaries},
language = {eng},
location = {Cambridge, UK},
isbn = {978-1-107-03379-5},
pages = {317-318},
publisher = {Cambridge University Press},
title = {Resonant switch model of twin peak HF QPOs applied to the atoll source 4U 1636-53 (Conference Paper)},
url = {https://arxiv.org/abs/1212.6669},
year = {2012}
}
TY - JOUR
ID - 42581
AU - Kotrlová, Andrea - Stuchlík, Zdeněk - Török, Gabriel
PY - 2012
TI - Resonant switch model of twin peak HF QPOs applied to the atoll source 4U 1636-53 (Conference Paper)
PB - Cambridge University Press
CY - Cambridge, UK
SN - 9781107033795
KW - Accretion
KW - Accretion disks
KW - Stars: neutron
KW - X-rays: binaries
UR - https://arxiv.org/abs/1212.6669
N2 - We present a Resonant Switch (RS) model of twin peak high-frequency quasi-periodic oscillations (HF QPOs), assuming switch of twin oscillations at a resonant point, where frequencies of the upper and lower oscillations ?U and ?L become to be 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 non-linear resonant phenomena. The RS model enables to determine range of allowed values of spin a and massM of the neutron star located at the atoll source 4U 1636-53 where two resonant points are observed at frequency ratios ?U : ?L = 3:2, 5:4.
ER -
KOTRLOVÁ, Andrea, Zdeněk STUCHLÍK a Gabriel TÖRÖK. Resonant switch model of twin peak HF QPOs applied to the atoll source 4U 1636-53 (Conference Paper). In \textit{Proceedings of the International Astronomical Union}. Cambridge, UK: Cambridge University Press. s.~317-318. ISBN~978-1-107-03379-5. doi:10.1017/S1743921312020194. 2012.
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