Oscillations of tori in the pseudo-Newtonian potential

@article{43300,
   author = {Šrámková, Eva},
   article_location = {FR - Francouzská republika},
   article_number = {únor 2007},
   doi = {http://dx.doi.org/10.1051/0004-6361:20065979},
   keywords = {accretion disks ? black hole physics},
   language = {eng},
   issn = {0004-6361},
   journal = {Astronomy & Astrophysics},
   title = {Oscillations of tori in the pseudo-Newtonian potential},
   volume = {467},
   year = {2007}
}

TY  - JOUR
ID  - 43300
AU  - Šrámková, Eva
PY  - 2007
TI  - Oscillations of tori in the pseudo-Newtonian potential
JF  - Astronomy & Astrophysics
VL  - 467
IS  - únor 2007
SP  - 641-646
EP  - 641-646
SN  - 00046361
KW  - accretion disks ? black hole physics
N2  - The high-frequency quasi-periodic oscillations (HF QPOs) in neutron star and stellar-mass black hole X-ray binaries may be the result of a resonance between the radial and vertical epicyclic oscillations in strong gravity. In this paper we investigate the resonant coupling between the epicyclic modes in a torus in a strong gravitational field. We perform numerical simulations of axisymmetric constant angular momentum tori in the pseudo-Newtonian potential.
ER  - 

ŠRÁMKOVÁ, Eva. Oscillations of tori in the pseudo-Newtonian potential. \textit{Astronomy \&{} Astrophysics}. FR - Francouzská republika, 2007, roč.~467, únor 2007, s.~641-646. ISSN~0004-6361. Dostupné z: https://dx.doi.org/10.1051/0004-6361:20065979.