The twin peak QPOs in neutron star and black hole

@article{42061,
   author = {Török, Gabriel},
   article_location = {MX - Spojené státy mexické},
   article_number = {říjen 2006},
   keywords = {Accretion discs, Black hole physics, hydrodynamics, neutron stars},
   language = {eng},
   issn = {0185-1101},
   journal = {Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias)},
   title = {The twin peak QPOs in neutron star and black hole},
   volume = {27},
   year = {2007}
}

TY  - JOUR
ID  - 42061
AU  - Török, Gabriel
PY  - 2007
TI  - The twin peak QPOs in neutron star and black hole
JF  - Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias)
VL  - 27
IS  - říjen 2006
SP  - 8-17
EP  - 8-17
SN  - 01851101
KW  - Accretion discs, Black hole physics, hydrodynamics, neutron stars
N2  - The resonance model proposed in 2000 by Kluzniak and Abramowicz, explains the twin peak, high frequency, quasi periodic oscillations (HF QPOs) observed in the X-ray flux from black hole and neutron stars, as a non-linear resonance in modes of oscillations of accretion flows in strong gravity. While several important physical questions remain unanswered, recent observations of HF QPOs provide direct evidence of non-linear resonances. This article gives an up to date (May 2006) review of what has been explained, and what has not been explained, by the resonance model.
ER  - 

TÖRÖK, Gabriel. The twin peak QPOs in neutron star and black hole. \textit{Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias)}. MX - Spojené státy mexické, 2007, roč.~27, říjen 2006, s.~8-17. ISSN~0185-1101.