Prediction of the Black-Hole Mass in 3C 273 by Multiband Observations
2003 ◽
Vol 214
◽
pp. 281-286
Keyword(s):
X Ray
◽
With the determined black-hole (BH) spin of 3C 273 by data-fitting to the detected iron Kα line emission in the soft X-ray band, the BH mass of the galaxy is predicted by formulations of both the observed disk-luminosity in the optical-UV band and the observed jet-precession in the radio band. The multiband synthesis suggests that the BH is supermassive, 2.4 × 109M⊙. Simultaneously, other physical parameters are self-consistently obtained at the precessing radius of 230.2rg: the accretion rate of the disk is 74.9M⊙ yr−1, the Shakura-Sunyaev viscosity α is 0.134, and the radial & orbital velocities of fluid elements are 4.3 × 10−8 and 6.6 × 10−2, respectively.
2012 ◽
Vol 8
(S290)
◽
pp. 373-374
Keyword(s):
2008 ◽
Vol 176
(2)
◽
pp. 355-373
◽