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Low-energy gamma rays from Cygnus X-1 (1985)

Roques, J. P. ; Paul, J. ; Mandrou, P. ; [et al.]

In: CASI

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Publication Date: 2019-06-28

Description: The Cyg X-1 was observed by the balloonborne telescope OPALE, in June 1976. The high energy spectrum of the source, which was in its superlow state, was seen to extend well beyond 1 MeV. The observed low energy gamma ray component of Cyg X-1 is compared with the predictions of recent models involving accretion onto a stellar black hole, and including a possible contribution from the pair annihilation 511 keV gamma ray line.

Keywords: SPACE RADIATION

Type: OG-2.4-13 , 19th Intern. Cosmic Ray Conf - Vol. 1; p 193-196; NASA-CP-2376-VOL-1

Format: application/pdf

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