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- W48763692 abstract "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 × 10 9 M ⊙ . Simultaneously, other physical parameters are self-consistently obtained at the precessing radius of 230.2 r g : the accretion rate of the disk is 74.9 M ⊙ 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." @default.
- W48763692 created "2016-06-24" @default.
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- W48763692 date "2003-01-01" @default.
- W48763692 modified "2023-09-26" @default.
- W48763692 title "Prediction of the Black-Hole Mass in 3C 273 by Multiband Observations" @default.
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- W48763692 doi "https://doi.org/10.1017/s0074180900194574" @default.
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