Epicyclic oscillation modes of a Newtonian, non-slender torus

@article{41404,
   author = {Šrámková, Eva},
   article_location = {WEINHEIM},
   article_number = {9},
   doi = {http://dx.doi.org/10.1002/asna.200510423},
   keywords = {black hole physics; X-ray variability},
   language = {eng},
   issn = {0004-6337},
   journal = {Astronomische Nachrichten},
   title = {Epicyclic oscillation modes of a Newtonian, non-slender torus},
   volume = {326},
   year = {2005}
}

TY  - JOUR
ID  - 41404
AU  - Šrámková, Eva
PY  - 2005
TI  - Epicyclic oscillation modes of a Newtonian, non-slender torus
JF  - Astronomische Nachrichten
VL  - 326
IS  - 9
SP  - 835-837
EP  - 835-837
PB  - WILEY-V C H VERLAG GMBH
SN  - 00046337
KW  - black hole physics
KW  - X-ray variability
N2  - All normal modes of oscillations of slender tori have been expressed analytically in the classic work by Blaes (1985). We adopt his approach in order to calculate the eigenfunctions and eigenfrequencies of a particular class of epicyclic modes for slightly non-slender tori, and present results of our numerical simulation of torus epicyclic modes of oscillations, which will be compared with the analytical results.
ER  - 

ŠRÁMKOVÁ, Eva. Epicyclic oscillation modes of a Newtonian, non-slender torus. \textit{Astronomische Nachrichten}. WEINHEIM: WILEY-V C H VERLAG GMBH, 2005, vol.~326, No~9, p.~835-837. ISSN~0004-6337. Available from: https://dx.doi.org/10.1002/asna.200510423.