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Impulsive Electromagnetic Emission near a Black Hole

  • Authors: Christopher Thompson

2019 The Astrophysical Journal 874 48.

  • Provider: AAS Journals

Caption: Figure 3.

Dependence of ray fluence on latitude above and below the equatorial caustic on the sphere at infinity, as see in Figure 2. BH spins range from a = 0 (black points) to a/M = 0.9 (red points). Angular dependence is ﹩| \theta -\pi /2{| }^{-1}﹩ in the simplest case of a nonspinning BH (dotted line).

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