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@inproceedings{42160,
author = {Abramowicz, Marek and Stuchlík, Zdeněk and Šrámková, Eva and Török, Gabriel and KLUŹNIAK, Włodek},
address = {Italy},
booktitle = {Proceedings of Science},
doi = {http://dx.doi.org/10.22323/1.033.0096},
keywords = {Black hole, neutron star, QPO, non-linear resoance},
language = {eng},
location = {Italy},
pages = {1-6},
publisher = {International School for Advanced Studies},
title = {Non-linear resonance model for black hole and neutron star QPOs: observation and theory},
year = {2006}
}
TY - JOUR
ID - 42160
AU - Abramowicz, Marek - Stuchlík, Zdeněk - Šrámková, Eva - Török, Gabriel - KLUŹNIAK, Włodek
PY - 2006
TI - Non-linear resonance model for black hole and neutron star QPOs: observation and theory
PB - International School for Advanced Studies
CY - Italy
KW - Black hole, neutron star, QPO, non-linear resoance
N2 - Kilohertz Quasi-Periodic Oscillations (QPOs) have been detected in many accreting X-ray binaries. It has been suggested that the kHz QPO frequencies observed in the modulation of the X-ray flux reflect a non-linear resonance between two modes of accreting disk oscillations. A 3:2 resonant ratio of frequencies has been clearly recognized in the black-hole QPO data supporting the non-linear resonance hypothesis. It is often discussed whether the same 3:2 ratio appears in case of the neutron star QPOs as well.
ER -
ABRAMOWICZ, Marek, Zdeněk STUCHLÍK, Eva ŠRÁMKOVÁ, Gabriel TÖRÖK a Włodek KLU$\backslash$'ZNIAK. Non-linear resonance model for black hole and neutron star QPOs: observation and theory. In \textit{Proceedings of Science}. Italy: International School for Advanced Studies, 2006, s.~1-6. Dostupné z: https://dx.doi.org/10.22323/1.033.0096.
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