Continuum reverberation mapping of accretion disks depending on the vertical structures in active galactic nuclei

Open Access

Fig. 1.

Calculated effective radius ratio, ℛ, taking α = 0.1, R_in = 3R_S and R_out = 5000R_S. In panel (a), we show ℛ with a given value of M_• but varying accretion rates. In panels (b) and (c), we fix $\dot{M}$ ${\dot{\mathscr{M}}}$ and alter M_•. Although the values of ℛ show complicated behaviors, the observed radii is 1.2–2.6 times of the blackbody ones overall.

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