Photon Bending Effects near Black Hole Horizons: Spectral and Timing Signatures

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

We will present the main spectral and timing features of X-ray radiation that can be seen in black hole systems only. We will demonstrate that the photon-electron interaction along with general relativistic effects lead to the formation of a characteristic spectrum. Photon bending of the upscattered photons near a black hole horizon results in a powerful pair outflow that can be responsible for the jet formation near black holes.

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