Determining the spin of two stellar-mass black holes from disc reflection signatures

作者：Reis R C^*; Fabian A C; Ross R R; Miller J M

来源：Monthly Notices of the Royal Astronomical Society, 2009, 395(3): 1257-1264.

DOI：10.1111/j.1365-2966.2009.14622.x

• accretion, accretion discs
• black hole physics
• X-rays: individual: J1753.5-0127, J1655-40

We present measurements of the dimensionless spin parameters and inner-disc inclination of two stellar-mass black holes. The spin parameter of SWIFT J1753.5-0127 and GRO J1655-40 is estimated by modelling the strong reflection signatures present in their XMM-Newton observations. Using a newly developed, self-consistent reflection model which includes the blackbody radiation of the disc as well as the effect of Comptonization, blurred with a relativistic line function, we infer the spin parameter of SWIFT J1753.5-0127 to be 0.76(-0.15)( 0.11). The inclination of this system is estimated at 55 degrees( 2)(7). For GROJ1655-40, we find that the disc is significantly misaligned to the orbital plane, with an innermost inclination of 30 degrees( 5)(10). Allowing the inclination to be a free parameter, we find a lower limit for the spin of 0.90, this value increases to that of a maximal rotating black hole when the inclination is set to that of the orbital plane of J1655-40. Our technique is independent of the black hole mass and distance, uncertainties in which are among the main contributors to the spin uncertainty in previous works.

• 出版日期2009-5-21