. . "Mass estimate of the XTE J1650-500 black hole from the Extended Orbital Resonance Model for high-frequency QPOs"@en . "XTE J1650-500 je galaktick\u00FD bin\u00E1rn\u00ED syst\u00E9m s \u010Dernou d\u00EDrou, pro n\u011Bj\u017E byla detekov\u00E1na alespo\u0148 jedna QPO na 250Hz. Krom\u011B toho existuj\u00ED n\u00E1znaky, \u017Ee syst\u00E9m obsahuje t\u00E9m\u011B\u0159 extr\u00E9mn\u00ED Kerrovu \u010Dernou d\u00EDru se spinem bl\u00EDzk\u00FDm 0.998 a hmotnost\u00ED M=0.9953; anal\u00FDza v lok\u00E1ln\u011B nerotuj\u00EDc\u00ED b\u00E1zi odhaluje hrb v bl\u00EDzkosti margin\u00E1ln\u011B stabiln\u00ED orbity. D\u00E1le bylo navr\u017Eeno, \u017Ee tento hrb by mohl excitovat epicyklick\u00FD pohyb \u010D\u00E1stic v bl\u00EDzkosti ISCO s frekvencemi typick\u00FDmi pro vysokofrekven\u010Dn\u00ED QPO. Charakteristick\u00E9 frekvence hrbem indukovan\u00FDch oscilac\u00ED byly definov\u00E1ny jako maximum kladn\u00E9 zm\u011Bny orbit\u00E1ln\u00ED rychlosti spojen\u00E9 s LNRF s vlastn\u00EDm polom\u011Brem."@cs . "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." . "0004-6361" . . . "RIV/47813059:19240/08:#0001922" . "Stuchl\u00EDk, Zden\u011Bk" . "Astronomy and Astrophysics" . . "Mass estimate of the XTE J1650-500 black hole from the Extended Orbital Resonance Model for high-frequency QPOs" . . . "RIV/47813059:19240/08:#0001922!RIV09-MSM-19240___" . "Mass estimate of the XTE J1650-500 black hole from the Extended Orbital Resonance Model for high-frequency QPOs" . . . "377845" . "000261431500005" . "Z(MSM4781305903)" . . "19240" . "Accretion, accretion discs, Black hole physics, Relativity, X-rays, individuals, XTE J1650-500"@en . . . "Odhad hmotnosti \u010Dern\u00E9 d\u00EDry XTE J1650-500 z roz\u0161\u00ED\u0159en\u00E9ho orbit\u00E1ln\u00EDho rezonan\u010Dn\u00EDho modelu pro vysokofrekven\u010Dn\u00ED QPO"@cs . . . "Mass estimate of the XTE J1650-500 black hole from the Extended Orbital Resonance Model for high-frequency QPOs"@en . "5"^^ . "492" . "2"^^ . . . "Slan\u00FD, Petr" . "Odhad hmotnosti \u010Dern\u00E9 d\u00EDry XTE J1650-500 z roz\u0161\u00ED\u0159en\u00E9ho orbit\u00E1ln\u00EDho rezonan\u010Dn\u00EDho modelu pro vysokofrekven\u010Dn\u00ED QPO"@cs . . "FR - Francouzsk\u00E1 republika" . "2"^^ . "1" . "[68619FA05E24]" . . . "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 . .