Figure 15 from Toward Determining the Number of Observable Supermassive Black Hole Shadows

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Toward Determining the Number of Observable Supermassive Black Hole Shadows

Authors: Dominic W. Pesce, Daniel C. M. Palumbo, Ramesh Narayan, Lindy Blackburn, Sheperd S. Doeleman, Michael D. Johnson, Chung-Pei Ma, Neil M. Nagar, Priyamvada Natarajan, and Angelo Ricarte

2021 The Astrophysical Journal 923 260.

Provider: AAS Journals

Caption: Figure 15.

The ratio of the bolometric luminosity L_bol to the accretion luminosity ﹩\dot{M}{c}^{2}﹩ versus the accretion rate ﹩\dot{m}﹩ and colored by SMBH mass m. The dashed gray line indicates the input radiative efficiency of η = 0.1; for ﹩{\dot{m}}_{0}\gtrsim {10}^{-2.5}﹩ the radiative efficiency of our model exceeds this input assumption.

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