Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aas...187.5802h&link_type=abstract
American Astronomical Society, 187th AAS Meeting, #58.02; Bulletin of the American Astronomical Society, Vol. 27, p.1368
Astronomy and Astrophysics
Astronomy
Scientific paper
Observations with the EGRET telescope on the Compton Observatory reveal the extensive, high-energy gamma ray emission which results from cosmic ray interactions with the photons and matter in the plane of the Galaxy. The study of this diffuse emission from the Galaxy, which is the most prominent feature of the high-energy gamma-ray sky, is expected to yield information about the production and distribution of cosmic rays in the Galaxy. In this paper we present spectra of the diffuse emission from the Galactic plane over the range 30--30,000 MeV, averaged over bins 10(deg) in longitude by 4(deg) in latitude. These spectra are compared with those predicted by the model of the diffuse gamma ray emission by Hunter et al. (1996, APJ) to verify the model and to assess the variation of the cosmic ray electron and proton densities across the Galaxy.
Bertsch David L.
Catelli Jennifer R.
Digel Seth William
Dingus Brenda Lynn
Esposito Joseph A.
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