A localized excess of diffuse gamma radiation

Astronomy and Astrophysics – Astronomy

Scientific paper

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Cosmic Rays, Diffuse Radiation, Galactic Structure, Gamma Ray Astronomy, Gamma Rays, H I Regions, Interstellar Matter, Radio Astronomy, Decimeter Waves, Density (Number/Volume), Gamma Ray Observatory, Ultrahigh Frequencies

Scientific paper

Using archival Energetic Gamma Ray Experiment Telescope (EGRET) gamma-ray data and atomic hydrogen (H I) column densities derived from 21 cm radio observations, we have found a large irregular region in the northern Galactic hemisphere extending from (l approximately 90 deg, b approximately 52 deg) to (l approximately 45 deg, b approximately 77 deg) with a significant enhancement in the gamma-ray emissivity compared to the surrounding sky. The region contains no previously identified gamma-ray point sources. The emission may arise from a localized enhancement in cosmic-ray density or from the presence of matter other than H I. If the emission is due to unseen matter, a column density enhancement equivalent to approximately 2 x 1020 H-atoms/sq cm is required.

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