Resonant switch model of twin peak HF QPOs applied to the atoll
source 4U 1636-53 (Conference Paper)

D 2012

Resonant switch model of twin peak HF QPOs applied to the atoll source 4U 1636-53 (Conference Paper)

KOTRLOVÁ, Andrea, Zdeněk STUCHLÍK a Gabriel TÖRÖK

Základní údaje

Originální název

Resonant switch model of twin peak HF QPOs applied to the atoll source 4U 1636-53 (Conference Paper)

Autoři

KOTRLOVÁ, Andrea, Zdeněk STUCHLÍK a Gabriel TÖRÖK

Vydání

Cambridge, UK, Proceedings of the International Astronomical Union, od s. 317-318, 2 s. 2012

Nakladatel

Cambridge University Press

Další údaje

Jazyk

angličtina

Typ výsledku

Stať ve sborníku

Obor

10308 Astronomy

Utajení

není předmětem státního či obchodního tajemství

Odkazy

URL

Organizační jednotka

Filozoficko-přírodovědecká fakulta v Opavě

ISBN

978-1-107-03379-5

ISSN

DOI

http://dx.doi.org/10.1017/S1743921312020194

Klíčová slova anglicky

Accretion; Accretion disks; Stars: neutron; X-rays: binaries

Štítky

FÚ, GA202-090772, GD205-09H033, sbornik

Příznaky

Mezinárodní význam

Návaznosti

GA202/09/0772, projekt VaV. GD205/09/H033, projekt VaV.

Změněno: 7. 4. 2021 11:55, Mgr. Pavlína Jalůvková

Anotace

V originále

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.

Citovat

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 Proceedings of the International Astronomical Union. Cambridge, UK: Cambridge University Press, 2012, s. 317-318. ISBN 978-1-107-03379-5. Dostupné z: https://dx.doi.org/10.1017/S1743921312020194.

@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, 2012, s.~317-318. ISBN~978-1-107-03379-5. Dostupné z: https://dx.doi.org/10.1017/S1743921312020194.

Podrobný výpis o publikaci