About: Disc-oscillation resonance and neutron star QPOs: 3:2 epicyclic orbital model     Goto   Sponge   NotDistinct   Permalink

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  • The high-frequency quasi-periodic oscillations (HF QPOs) that appear in the X-ray fluxes of low-mass X-ray binaries remain an unexplained phenomenon. Among other ideas, it has been suggested that a non-linear resonance between two oscillation modes in an accretion disc orbiting either a black hole or a neutron star plays a role in exciting the observed modulation. Several possible resonances have been discussed. A particular model assumes resonances in which the disc-oscillation modes have the eigenfrequencies equal to the radial and vertical epicyclic frequencies of geodesic orbital motion. This model has been discussed for black hole microquasar sources as well as for a group of neutron star sources.
  • The high-frequency quasi-periodic oscillations (HF QPOs) that appear in the X-ray fluxes of low-mass X-ray binaries remain an unexplained phenomenon. Among other ideas, it has been suggested that a non-linear resonance between two oscillation modes in an accretion disc orbiting either a black hole or a neutron star plays a role in exciting the observed modulation. Several possible resonances have been discussed. A particular model assumes resonances in which the disc-oscillation modes have the eigenfrequencies equal to the radial and vertical epicyclic frequencies of geodesic orbital motion. This model has been discussed for black hole microquasar sources as well as for a group of neutron star sources. (en)
Title
  • Disc-oscillation resonance and neutron star QPOs: 3:2 epicyclic orbital model
  • Disc-oscillation resonance and neutron star QPOs: 3:2 epicyclic orbital model (en)
skos:prefLabel
  • Disc-oscillation resonance and neutron star QPOs: 3:2 epicyclic orbital model
  • Disc-oscillation resonance and neutron star QPOs: 3:2 epicyclic orbital model (en)
skos:notation
  • RIV/47813059:19240/10:#0002992!RIV11-MSM-19240___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(GA202/09/0772), P(LC06014), Z(MSM4781305903)
http://linked.open...iv/cisloPeriodika
  • A72
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 254577
http://linked.open...ai/riv/idVysledku
  • RIV/47813059:19240/10:#0002992
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • QUASI-PERIODIC OSCILLATIONS, HIGH-FREQUENCY QPOS, X-RAY BINARIES, INTEGRATED RELATIVISTIC TORI, EQUATION-OF-STATE, SOURCE 4U 1636-53, BLACK-HOLE SPIN, KHZ QPOS, KILOHERTZ QPOS, SLENDER TORI (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • FR - Francouzská republika
http://linked.open...ontrolniKodProRIV
  • [999353FFBECC]
http://linked.open...i/riv/nazevZdroje
  • Astronomy & 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
  • 522
http://linked.open...iv/tvurceVysledku
  • Stuchlík, Zdeněk
  • Török, Gabriel
  • Čech, Petr
  • Šrámková, Eva
  • Urbanec, Martin
  • Bakala, Pavel
http://linked.open...n/vavai/riv/zamer
issn
  • 0004-6361
number of pages
http://localhost/t...ganizacniJednotka
  • 19240
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