About: Mass estimate of the XTE J1650-500 black hole from the Extended Orbital Resonance Model for high-frequency QPOs     Goto   Sponge   Distinct   Permalink

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  • XTE J1650-500 is a Galactic black-hole binary system for which at least one high-frequency QPO at 250Hz was reported. Moreover there are indications that the system harbours a near-extreme Kerr black-hole with the spin near 0.998 and mass M0.9953, being analyzed in the locally non-rotating frames, reveals a hump near the marginally stable orbit. Further it was suggested that the hump could excite the epicyclic motion of particles near the ISCO with frequencies typical for high-frequency QPOs. Characteristic frequency of the hump-induced oscillations was defined as the maximal positive rate of change of the LNRF-related orbital velocity with the proper radial distance.
  • XTE J1650-500 is a Galactic black-hole binary system for which at least one high-frequency QPO at 250Hz was reported. Moreover there are indications that the system harbours a near-extreme Kerr black-hole with the spin near 0.998 and mass M0.9953, being analyzed in the locally non-rotating frames, reveals a hump near the marginally stable orbit. Further it was suggested that the hump could excite the epicyclic motion of particles near the ISCO with frequencies typical for high-frequency QPOs. Characteristic frequency of the hump-induced oscillations was defined as the maximal positive rate of change of the LNRF-related orbital velocity with the proper radial distance. (en)
  • XTE J1650-500 je galaktický binární systém s černou dírou, pro nějž byla detekována alespoň jedna QPO na 250Hz. Kromě toho existují náznaky, že systém obsahuje téměř extrémní Kerrovu černou díru se spinem blízkým 0.998 a hmotností M=0.9953; analýza v lokálně nerotující bázi odhaluje hrb v blízkosti marginálně stabilní orbity. Dále bylo navrženo, že tento hrb by mohl excitovat epicyklický pohyb částic v blízkosti ISCO s frekvencemi typickými pro vysokofrekvenční QPO. Charakteristické frekvence hrbem indukovaných oscilací byly definovány jako maximum kladné změny orbitální rychlosti spojené s LNRF s vlastním poloměrem. (cs)
Title
  • Mass estimate of the XTE J1650-500 black hole from the Extended Orbital Resonance Model for high-frequency QPOs
  • Mass estimate of the XTE J1650-500 black hole from the Extended Orbital Resonance Model for high-frequency QPOs (en)
  • Odhad hmotnosti černé díry XTE J1650-500 z rozšířeného orbitálního rezonančního modelu pro vysokofrekvenční QPO (cs)
skos:prefLabel
  • Mass estimate of the XTE J1650-500 black hole from the Extended Orbital Resonance Model for high-frequency QPOs
  • Mass estimate of the XTE J1650-500 black hole from the Extended Orbital Resonance Model for high-frequency QPOs (en)
  • Odhad hmotnosti černé díry XTE J1650-500 z rozšířeného orbitálního rezonančního modelu pro vysokofrekvenční QPO (cs)
skos:notation
  • RIV/47813059:19240/08:#0001922!RIV09-MSM-19240___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • Z(MSM4781305903)
http://linked.open...iv/cisloPeriodika
  • 1
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
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http://linked.open...iv/duvernostUdaju
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http://linked.open...dnocenehoVysledku
  • 377845
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  • RIV/47813059:19240/08:#0001922
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  • Accretion, accretion discs, Black hole physics, Relativity, X-rays, individuals, XTE J1650-500 (en)
http://linked.open.../riv/klicoveSlovo
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  • FR - Francouzská republika
http://linked.open...ontrolniKodProRIV
  • [68619FA05E24]
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  • Astronomy and Astrophysics
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 492
http://linked.open...iv/tvurceVysledku
  • Stuchlík, Zdeněk
  • Slaný, Petr
http://linked.open...ain/vavai/riv/wos
  • 000261431500005
http://linked.open...n/vavai/riv/zamer
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  • 0004-6361
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  • 19240
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