Gamma rays from Cygnus X-1: Modeling and nonthermal pair production
Description:
The gamma-ray bump observed between 0.5 and 2 MeV in the spectrum of Cygnus X-1 can be interpreted as the thermal emissions from a hot (kT)approximately)400 keV) pair-dominated cloud. We argue that the X-rays and gamma rays are produced in separate emission regions, and calculate the photon-photon pair production rate from X-ray and gamma-ray interactions in the vicinity of Cyg X-1 by employing a simplified geometry for the two emitting regions.
Date:
February 1, 1988
Creator:
Dermer, C. D. & Liang, E. P.
Item Type:
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