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The e+–e− Annihilation Line and the Cosmic X-Ray Background
Published online by Cambridge University Press: 04 August 2017
Abstract
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The possibility that the processes responsible for the Cosmic X-ray Background (CXB) would also produce an e−-e+ annihilation feature is examined. Under the assumption that these processes are thermal, the absence of a strong e−-e+ annihilation feature places constraints on the compactness (L/R ratio) of these sources. Observations favor sources of small compactness ratio.
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- Research Article
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- Copyright © Reidel 1983
References
Marshall, F., Boldt, E., Holt, S., Miller, R., Mushotzky, R., Rose, L. A., Rothchild, R. and Serlemitsos, P., 1980, Ap. J., 235, 377.Google Scholar
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