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  • V Galaktických mikrokvasarech s dvojitými kHz kvaziperiodickými oscilacemi (QPO) je poměr frekvencí píků 3:2. To podporuje hypotézu, že dvojité kHz QPO jsou způsobeny nelineární rezonancí mezi dvěma mody oscilací akrečního disku. Pro mikrokvasary se známou hmotností stručně porovnáváme odhady spinu černé díry založené na modelu orbitální rezonance s nedávno oznámenými přepověďmi spinu získanými fitováním spektrálního kontinua. (cs)
  • In the Galactic microquasars with double peak kHz quasi-periodic oscillations (QPOs), the ratio of the two frequencies is 3:2. This supports the suggestion that double peak kHz QPOs are due to a non-linear resonance between two modes of accretion disk oscillations. For the microquasars with known mass, we briefly compare the black hole spin estimates based on the orbital resonance model with the recently reported spin predictions obtained by fitting the spectral continua.
  • In the Galactic microquasars with double peak kHz quasi-periodic oscillations (QPOs), the ratio of the two frequencies is 3:2. This supports the suggestion that double peak kHz QPOs are due to a non-linear resonance between two modes of accretion disk oscillations. For the microquasars with known mass, we briefly compare the black hole spin estimates based on the orbital resonance model with the recently reported spin predictions obtained by fitting the spectral continua. (en)
Title
  • QPOs in microquasars: the spin problem
  • QPO v mikrokvasarech: problém spinu (cs)
  • QPOs in microquasars: the spin problem (en)
skos:prefLabel
  • QPOs in microquasars: the spin problem
  • QPO v mikrokvasarech: problém spinu (cs)
  • QPOs in microquasars: the spin problem (en)
skos:notation
  • RIV/47813059:19240/06:#0000815!RIV08-MSM-19240___
http://linked.open.../vavai/riv/strany
  • 119-121
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • Z(MSM4781305903)
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
  • 496135
http://linked.open...ai/riv/idVysledku
  • RIV/47813059:19240/06:#0000815
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • Black hole physics, X-rays: binaries (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...ontrolniKodProRIV
  • [DF1369E87E33]
http://linked.open...v/mistoKonaniAkce
  • Praha
http://linked.open...i/riv/mistoVydani
  • Cambridge
http://linked.open...i/riv/nazevZdroje
  • Binary Stars as Critical Tools and Tests in Contemporary Astrophysics
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...UplatneniVysledku
http://linked.open...iv/tvurceVysledku
  • Stuchlík, Zdeněk
  • Török, Gabriel
  • Šrámková, Eva
  • Abramowicz, Marek
http://linked.open...vavai/riv/typAkce
http://linked.open.../riv/zahajeniAkce
http://linked.open...n/vavai/riv/zamer
number of pages
http://purl.org/ne...btex#hasPublisher
  • Cambridge University Press
https://schema.org/isbn
  • 978-0-521-863-483
http://localhost/t...ganizacniJednotka
  • 19240
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