Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...445l.109c&link_type=abstract
Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 445, no. 2, p. L109-L112
Astronomy and Astrophysics
Astronomy
8
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.
Chen Aiqing
Dwyer Joseph
Kaaret Phil
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