Spectral signature of oscillating slender tori surrounding Kerr black holes

@article{42726,
   author = {Abramowicz, Marek and Bakala, Pavel and Török, Gabriel and Kluźniak, Włodek and Mazur, G. P. and Straub, Odele and Vincent, Frédéric H.},
   article_location = {FR - Francouzská republika},
   article_number = {March},
   doi = {http://dx.doi.org/10.1051/0004-6361/201323103},
   keywords = {accretion, accretion disks; black hole physics; relativistic processes},
   language = {eng},
   issn = {0004-6361},
   journal = {Astronomy & Astrophysics},
   title = {Spectral signature of oscillating slender tori surrounding Kerr black holes},
   url = {http://www.aanda.org/articles/aa/abs/2014/03/aa23103-13/aa23103-13.html},
   volume = {563},
   year = {2014}
}

TY  - JOUR
ID  - 42726
AU  - Abramowicz, Marek - Bakala, Pavel - Török, Gabriel - Kluźniak, Włodek - Mazur, G. P. - Straub, Odele - Vincent, Frédéric H.
PY  - 2014
TI  - Spectral signature of oscillating slender tori surrounding Kerr black holes
JF  - Astronomy & Astrophysics
VL  - 563
IS  - March
SP  - "A109 - 1"-"A109 - 8"
EP  - "A109 - 1"-"A109 - 8"
SN  - 00046361
KW  - accretion, accretion disks
KW  - black hole physics
KW  - relativistic processes
UR  - http://www.aanda.org/articles/aa/abs/2014/03/aa23103-13/aa23103-13.html
N2  - Context. Some microquasars exhibit millisecond quasi-periodic oscillations (QPO) that are most probably related to phenomena occuring in the immediate vicinity of central black holes. Oscillations of accretion tori have been proposed to model these QPOs.Aims. Here, we aim at determining the observable spectral signature of slender accretion tori surrounding Kerr black holes. We analyse the impact of the inclination and spin parameters on the power spectra. Methods. Ray-traced power spectra of slender tori oscillation modes are computed in the Kerr metric. Results. We show that the power spectral densities of oscillating tori are very sensitive to the inclination and spin parameters. This strong dependency of the temporal spectra on inclination and spin may lead to observable constraints of these parameters. Conclusions. This work goes a step further in the analysis of the oscillating torus QPO model. It is part of a long-term study that will ultimately lead to comparison with observed
ER  - 

ABRAMOWICZ, Marek, Pavel BAKALA, Gabriel TÖRÖK, Włodek KLU$\backslash$'ZNIAK, G. P. MAZUR, Odele STRAUB a Frédéric H. VINCENT. Spectral signature of oscillating slender tori surrounding Kerr black holes. \textit{Astronomy \&{} Astrophysics}. FR - Francouzská republika, 2014, roč.~563, March, s.~''A109 - 1''-''A109 - 8'', 8 s. ISSN~0004-6361. Dostupné z: https://dx.doi.org/10.1051/0004-6361/201323103.