COS-B measurements of high-latitude gamma rays and evidence for a component not related to the gas

Details COS-B measurements of high-latitude gamma rays and evidence for a component not related to the gas COS-B measurements of high-latitude gamma rays and evidence for a component not related to the gas

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....9...90s&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Late Papers. Volume 9 (A85-22801 0

Astronomy and Astrophysics

Astronomy

Cosmic Gases, Gamma Ray Spectra, Milky Way Galaxy, Radiant Flux Density, Radiation Measurement, Spaceborne Astronomy, Compton Effect, Cos-B Satellite, Diffuse Radiation, Inverse Scattering, Particle Interactions

Scientific paper

The gamma ray latitude distribution for absolute value of b between 10 deg and 90 deg measured by COS-B is compared with the expected emission from cosmic-ray/gas interactions. An additional component is found which is unrelated to the gas, and which may be interpreted as a gamma-ray 'halo'. The possibility of an inverse-Compton origin is discussed using diffuse X-ray data.

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