. "2005-01-01+01:00"^^ . . "Model neline\u00E1rn\u00EDch rezonanc\u00ED pro QPOs u \u010Dern\u00FDch d\u011Br a neutronov\u00FDch hv\u011Bzd: teorie podpo\u0159ena pozorov\u00E1n\u00EDm"@cs . "463693" . "Z(MSM4781305903)" . . . "Model neline\u00E1rn\u00EDch rezonanc\u00ED pro QPOs u \u010Dern\u00FDch d\u011Br a neutronov\u00FDch hv\u011Bzd: teorie podpo\u0159ena pozorov\u00E1n\u00EDm"@cs . "Kluzniak, W." . "Relativity and gravitation, X-ray binaries, time variability"@en . "American Institute of Physics" . "Stuchl\u00EDk, Zden\u011Bk" . "A non-linear resonance model for the black hole and neutron star QPOs: theory supported by observations"@en . "A33-A33" . . "A non-linear resonance model for the black hole and neutron star QPOs: theory supported by observations"@en . . "1"^^ . "Kilohertz Quasi-Periodic Oscillations (QPOs) have been detected in many accreting X-ray binaries. It has been suggested that the highest QPO frequencies observed in the modulation of the X-ray flux reflect a non-linear resonance between two modes of accreting disk oscillation. This hypothesis implies certain very general predictions, several of which have been borne out by observations. Some of these follow from properties of non-linear oscillators, while the others are specific to oscillations of fluid in strong gravity. A 3:2 resonant ratio of frequencies can be clearly recognized in the black-hole as well as in the neutron-star QPO data."@en . . "Albert Einstein Century International Conference" . . "A non-linear resonance model for the black hole and neutron star QPOs: theory supported by observations" . "3"^^ . . "Kilohertz Quasi-Periodic Oscillations (QPOs) have been detected in many accreting X-ray binaries. It has been suggested that the highest QPO frequencies observed in the modulation of the X-ray flux reflect a non-linear resonance between two modes of accreting disk oscillation. This hypothesis implies certain very general predictions, several of which have been borne out by observations. Some of these follow from properties of non-linear oscillators, while the others are specific to oscillations of fluid in strong gravity. A 3:2 resonant ratio of frequencies can be clearly recognized in the black-hole as well as in the neutron-star QPO data." . "4"^^ . . "A non-linear resonance model for the black hole and neutron star QPOs: theory supported by observations" . "[8994581F2510]" . "RIV/47813059:19240/06:#0000105" . . "Paris" . . "978-0-7354-0359-8" . "19240" . "T\u00F6r\u00F6k, Gabriel" . "Abramowicz, Marek" . . . "United States of America" . "RIV/47813059:19240/06:#0000105!RIV07-MSM-19240___" . . "Kilohertzov\u00E9 kvaziperiodick\u00E9 oscilace (QPOs) byly detekov\u00E1ny v mnoha akre\u010Dn\u00EDch bin\u00E1rn\u00EDch syst\u00E9mech generuj\u00EDc\u00EDch rentgenovsk\u00E9 paprsky. Bylo navr\u017Eeno, \u017Ee nejvy\u0161\u0161\u00ED QPO frekvence pozorovan\u00E9 v modulaci toku rentgenovsk\u00E9ho z\u00E1\u0159en\u00ED reflektuj\u00ED neline\u00E1rn\u00ED rezonanci mezi dv\u011Bma mody oscilac\u00ED akre\u010Dn\u00EDho disku. Tato hypot\u00E9za implikuje jist\u00E9 velice obecn\u00E9 p\u0159edpov\u011Bdi inspirovan\u00E9 pozorov\u00E1n\u00EDm. N\u011Bkter\u00E9 z nich plynou z vlastnost\u00ED neline\u00E1rn\u00EDch oscil\u00E1tor\u016F, jin\u00E9 jsou specifick\u00E9 pro oscilace kapaliny siln\u00FDch gravita\u010Dn\u00EDch pol\u00ED. Rezonan\u010Dn\u00ED pom\u011Br 3:2 se jasn\u011B projevuje v datech pozorovan\u00FDch v syst\u00E9mech s \u010Dern\u00FDmi d\u011Brami i neutronov\u00FDmi hv\u011Bzdami."@cs . . . .