TY - JOUR
T1 - Galactic X Rays and Gamma Rays
AU - Cowsik, R.
AU - Pal, Yash
PY - 1969
Y1 - 1969
N2 - 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.
AB - 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.
UR - https://www.scopus.com/pages/publications/0014656437
U2 - 10.1103/PhysRevLett.23.1467
DO - 10.1103/PhysRevLett.23.1467
M3 - Article
AN - SCOPUS:0014656437
SN - 0031-9007
VL - 23
SP - 1467
EP - 1468
JO - Physical Review Letters
JF - Physical Review Letters
IS - 25
ER -