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Description
  • 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 data.
  • 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 data. (en)
Title
  • Spectral signature of oscillating slender tori surrounding Kerr black holes
  • Spectral signature of oscillating slender tori surrounding Kerr black holes (en)
skos:prefLabel
  • Spectral signature of oscillating slender tori surrounding Kerr black holes
  • Spectral signature of oscillating slender tori surrounding Kerr black holes (en)
skos:notation
  • RIV/47813059:19240/14:#0005077!RIV15-MSM-19240___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • I, P(EE2.3.20.0071), P(GPP209/12/P740), S
http://linked.open...iv/cisloPeriodika
  • March
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
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http://linked.open...dnocenehoVysledku
  • 46572
http://linked.open...ai/riv/idVysledku
  • RIV/47813059:19240/14:#0005077
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • accretion, accretion disks; black hole physics; relativistic processes (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • FR - Francouzská republika
http://linked.open...ontrolniKodProRIV
  • [913595056AEB]
http://linked.open...i/riv/nazevZdroje
  • Astronomy and Astrophysics
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 563
http://linked.open...iv/tvurceVysledku
  • Török, Gabriel
  • Bakala, Pavel
  • Mazur, G. P.
  • Abramowicz, Marek Artur
  • Kluźniak, Włodek
  • Vincent, Frédéric H.
  • Straub, Odele
http://linked.open...ain/vavai/riv/wos
  • 000333798000109
issn
  • 0004-6361
number of pages
http://bibframe.org/vocab/doi
  • 10.1051/0004-6361/201323103
http://localhost/t...ganizacniJednotka
  • 19240
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