Non-linear resonance model for black hole and neutron star QPOs: observation and theory

@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 and 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, p.~1-6. Available from: https://dx.doi.org/10.22323/1.033.0096.