GALACTIC X-RAYS AND GAMMA-RAYS

被引:6
作者
COWSIK, R
PAL, Y
机构
[1] Tata Institute of Fundamental Research
关键词
D O I
10.1103/PhysRevLett.23.1467
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
A consistent explanation of the observed galactic flux of high-energy γ rays and the reported galactic x-ray flux is provided in terms of Compton scattering of cosmic-ray electrons with the submillimeter radiation observed recently. It is predicted that the flux of galactic x rays, relative to that of cosmic x rays, will increase with increasing energy. Thus, if an increased enhancement in the flux of high-energy (∼200-keV) x rays in going across the galactic equator is not observed, the existence, on a galactic scale, of the submillimeter radiation will be ruled out. © 1969 The American Physical Society.
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页码:1467 / &
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