A note on the slope-shift anticorrelation in the neutron star kHz QPOs data

@inproceedings{42052,
   author = {Abramowicz, Marek and Török, Gabriel},
   address = {Opava},
   booktitle = {Proceedings of RAGtime 6/7: Workshops on black holes and neutron stars},
   keywords = {LMXRB, neutron stars, X-ray variability, observations, theory},
   language = {eng},
   location = {Opava},
   isbn = {80-7248-334-X},
   pages = {1-9},
   publisher = {Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, Ústav fyziky},
   title = {A note on the slope-shift anticorrelation in the neutron star kHz QPOs data},
   year = {2005}
}

TY  - JOUR
ID  - 42052
AU  - Abramowicz, Marek - Török, Gabriel
PY  - 2005
TI  - A note on the slope-shift anticorrelation in the neutron star kHz QPOs data
PB  - Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, Ústav fyziky
CY  - Opava
SN  - 807248334X
KW  - LMXRB, neutron stars, X-ray variability, observations, theory
N2  - Observations show that the upper and lower of the "twin peak" high frequency QPOs in neutron star sources very along lines in a frequency-frequency plot, and that their ratios cluster near the value 3/2. This behaviour is well consistent with the predictions of the non-linear resonance model for QPOs. In this Note, we further explore our recent finding that the coefficients A, B of the frequency-frequency lines for individual sources are anticorrelated. In the (A, B) plane, they occupy rather a narrow region along the line A = 3/2 - B/600 Hz. We show that this observational property of QPOs also follows from the resonance model.
ER  - 

ABRAMOWICZ, Marek a Gabriel TÖRÖK. A note on the slope-shift anticorrelation in the neutron star kHz QPOs data. In \textit{Proceedings of RAGtime 6/7: Workshops on black holes and neutron stars}. Opava: Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, Ústav fyziky, 2005, s.~1-9. ISBN~80-7248-334-X.