Cowsik, R. ; Pal, Yash (1969) Possible origin of high-energy cosmic gamma rays? Physical Review Letters, 22 (11). pp. 550-551. ISSN 0031-9007
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Official URL: http://prl.aps.org/abstract/PRL/v22/i11/p550_1
Related URL: http://dx.doi.org/10.1103/PhysRevLett.22.550
Abstract
The intensity of the new microwave radiation observed by Shivanandan, Houck, and Harwit is adequate to produce, by Compton scattering on cosmic-ray electrons, the flux and distribution of ~100-MeV γ rays reported by Clark, Garmire, and Kraushaar.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to American Physical Society. |
| ID Code: | 20690 |
| Deposited On: | 20 Nov 2010 13:43 |
| Last Modified: | 28 May 2011 10:27 |
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