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Fig. 7.

image

Lense-Thirring precession period compared to the potential co-moving precession period of the inner jet of TXS 0506+056 (green solid line; PLT = Pdisk = 7.48 yr). The bottom axis represents the black hole spin value from the maximally retrograde (a = −1) to maximally prograde (a = 1). Different lines represent the Lense-Thirring precession period for different slopes of the surface density profile of the inner accretion disk, using the notation Σ ∝ rs. Left panel: outer radius is , where rms is the marginally stable radius, which depends on the spin value. Middle panel: . Right panel: .

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