Comparison of far-infrared radiation with gamma radiation Large-scale structure of the galaxy

Details Comparison of far-infrared radiation with gamma radiation Large-scale structure of the galaxy Comparison of far-infrared radiation with gamma radiation Large-scale structure of the galaxy

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ssrv...36..285o&link_type=abstract

(International Astronomical Union, Meeting on Galactic Astrophysics and Gamma-Ray Astronomy, Patras, Greece, Aug. 19, 1982) Spac

Astronomy and Astrophysics

Astronomy

Far Infrared Radiation, Galactic Nuclei, Galactic Structure, Gamma Rays, Milky Way Galaxy, Cos-B Satellite, Cosmic Rays, Distribution (Property), Interstellar Gas, Particle Interactions, Spaceborne Astronomy

Scientific paper

The gamma-ray emissivity for the narrow component (FWHM = 2°) at the 0.3 - 5 GeV range is derived as a function of the galactocentric distance. The narrow component might result from the interaction between cosmic rays and H2 gas. The mass of gas in the Galactic Center is not large enough to produce the gamma-ray peak, but enough to produce the far-infrared peak. The relation of far-infrared dip and near-infrared hump near l = 356° to gamma-ray hump is discussed.

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