Mass of intermediate black hole in the source M82 X-1 restricted by models of twin high-frequency ...

@article{46127,
   author = {Kološ, Martin and Stuchlík, Zdeněk},
   article_location = {GB - Spojené království Velké Británie a},
   article_number = {3},
   doi = {http://dx.doi.org/10.1093/mnras/stv1120},
   keywords = {black hole physic; X-rays: individual: M82 X-1},
   language = {eng},
   issn = {0035-8711},
   journal = {Monthly Notices of the Royal Astronomical Society},
   title = {Mass of intermediate black hole in the source M82 X-1 restricted by models of twin high-frequency quasi-periodic oscillations},
   volume = {451},
   year = {2015}
}

TY  - JOUR
ID  - 46127
AU  - Kološ, Martin - Stuchlík, Zdeněk
PY  - 2015
TI  - Mass of intermediate black hole in the source M82 X-1 restricted by models of twin high-frequency quasi-periodic oscillations
JF  - Monthly Notices of the Royal Astronomical Society
VL  - 451
IS  - 3
SP  - 2575-2588
EP  - 2575-2588
SN  - 00358711
KW  - black hole physic
KW  - X-rays: individual: M82 X-1
N2  - We apply the relativistic precession (RP) model with its variants and the resonance epicyclic model with its variants, based on the frequencies of the geodesic epicyclic motion in the field of a Kerr black hole, to put limits on the mass of the black hole in the ultraluminous X-ray source M82 X-1 demonstrating twin high-frequency quasi-periodic oscillations (HF QPOs) with the frequency ratio near 3:2. The mass limits implied by the geodesic HF QPO models are compared to those obtained due to the model of string loop oscillations around a stable equilibrium position. Assuming the whole range of the black hole dimensionless spin, 0 < a < 1, the restrictions on the black hole mass related to the twin HF QPOs are widely extended and strongly model dependent; nevertheless, they give the lower limit M_{M82 (X-1)} > 130 M_{circle dot} confirming existence of an intermediate black hole in the M82 X-1 source. The upper limit given by one of the variants of the geodesic twin HF QPO models goes u
ER  - 

KOLOŠ, Martin and Zdeněk STUCHLÍK. Mass of intermediate black hole in the source M82 X-1 restricted by models of twin high-frequency quasi-periodic oscillations. \textit{Monthly Notices of the Royal Astronomical Society}. GB - Spojené království Velké Británie a, 2015, vol.~451, No~3, p.~2575-2588. ISSN~0035-8711. Available from: https://dx.doi.org/10.1093/mnras/stv1120.