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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 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.
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