Possible Origin of High-Energy Cosmic Gamma Rays?

R. Cowsik and Yash Pal
Phys. Rev. Lett. 22, 550 – Published 17 March 1969
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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.

  • Received 17 December 1969

DOI:https://doi.org/10.1103/PhysRevLett.22.550

©1969 American Physical Society

Authors & Affiliations

R. Cowsik and Yash Pal

  • Tata Institute of Fundamental Research, Bombay, 5, India

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Issue

Vol. 22, Iss. 11 — 17 March 1969

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