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Ultra-high-energy cosmic rays in the Magellanic Clouds
Published online by Cambridge University Press: 19 July 2016
Abstract
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Ultra-high-energy (UHE) γ-rays have been detected from several X-ray binaries. UHE γ-rays from sources in the LMC will interact in the microwave background producing electrons which emit synchrotron radiation in the X-ray and γ-ray bands. This radiation might be observable.
- Type
- The Interstellar Medium
- Information
- Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 432 - 433
- Copyright
- Copyright © Kluwer 1991
References
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Spicker, J. and Feitzinger, J.W. (1987),
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