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@article{44223,
author = {Slaný, Petr and Stuchlík, Zdeněk},
article_location = {FR - Francouzská republika},
article_number = {2},
doi = {http://dx.doi.org/10.1051/0004-6361:200810334},
keywords = {Accretion, accretion discs, Black hole physics, Relativity, X-rays, individuals, XTE J1650-500},
language = {eng},
issn = {0004-6361},
journal = {Astronomy & Astrophysics},
title = {Mass estimate of the XTE J1650-500 black hole from the Extended Orbital Resonance Model for high-frequency QPOs},
volume = {492},
year = {2008}
}
TY - JOUR
ID - 44223
AU - Slaný, Petr - Stuchlík, Zdeněk
PY - 2008
TI - Mass estimate of the XTE J1650-500 black hole from the Extended Orbital Resonance Model for high-frequency QPOs
JF - Astronomy & Astrophysics
VL - 492
IS - 2
SP - 319-322
EP - 319-322
SN - 00046361
KW - Accretion, accretion discs, Black hole physics, Relativity, X-rays, individuals, XTE J1650-500
N2 - 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, beinganalyzed 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.
ER -
SLANÝ, Petr a Zdeněk STUCHLÍK. Mass estimate of the XTE J1650-500 black hole from the Extended Orbital Resonance Model for high-frequency QPOs. \textit{Astronomy \&{} Astrophysics}. FR - Francouzská republika, 2008, roč.~492, č.~2, s.~319-322, 5 s. ISSN~0004-6361. Dostupné z: https://dx.doi.org/10.1051/0004-6361:200810334.
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