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In the presence of a black hole, light sources connect to observers along multiple paths.
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C. F. Gammie, J. C. McKinney, and G. Tóth, “HARM: A Numerical Scheme for General Relativistic Magnetohydrodynamics,” ApJ 589
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I. V. Igumenshchev, R. Narayan, and M. A. Abramowicz, “Three-dimensional Magnetohydrodynamic Simulations of Radiatively Inefficient Accretion Flows,” ApJ 592
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R. Takahashi, “Shapes and positions of black hole shadows in accretion disks and spin parameters of black holes,” ApJ 611
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