Intensities of inverse Compton gamma-rays in Galactic medium latitude.

Details Intensities of inverse Compton gamma-rays in Galactic medium latitude. Intensities of inverse Compton gamma-rays in Galactic medium latitude.

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995hepnp..19..974z&link_type=abstract

High Energ. Phys. Nucl. Phys., Vol. 19, No. 11, p. 974 - 979

Physics

Galaxy: Cosmic Rays, Galaxy: Gamma Rays

Scientific paper

The gamma-ray emissivity q/4π of galactic cosmic rays interacting with interstellar gases at medium-latitude (|b| = 10° - 20°) is determined by using recent EGRET data. A gamma-ray data method is used to obtain the emissivity. The inverse Compton (IC) integral intensities as a function of galactic longitude are obtained. The differential IC intensities averaged over all galactic longitudes are given.

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