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Relationship between the galactic matter distribution, cosmic-ray dynamics, and gamma-ray production

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/155411· OSTI ID:7214303
Theoretical considerations and analysis of the results of ..gamma..-ray astronomy suggest that the galactic cosmic rays are dynamically coupled to the interstellar matter through the magnetic fields; hence the the cosmic-ray density should be enhanced where the matter density is greatest on the scale of galactic arms. This concept has been explored in a galactic model using recent 21 cm radio observations of neutral hydrogen and 2.6 mm observations of carbon monoxide, which is considered to be a tracer of molecular hydrogen. The model assumes that (1) cosmic rays are galactic and not universal; (2) on the scale of galactic arms, the cosmic-ray column (surface) density is proportional to the total interstellar-gas column density; (3) the cosmic-ray scale height is significantly larger than the scale height of the matter; and (4) ours is a spiral galaxy characterized by an arm-to-interarm density ratio of about 3:1. The second assumption implies that the ..gamma..-ray emission is proportional to the square of the mass on the scale of galactic arms. The theoretical predictions for ..gamma..-rays produced by matter--cosmic-ray interactions in this model show a good correlation with the galactic ..gamma..-ray observations, not only in terms of the absolute intensities along the galactic plane but also in terms of the positions of specific galactic features near longitudes 315/sup 0/, 330/sup 0/--335/sup 0/, 340/sup 0/--345/sup 0/, 0/sup 0/, 25/sup 0/,and 35/sup 0/.
Research Organization:
NASA/Goddard Space Flight Center, Greenbelt, Maryland
OSTI ID:
7214303
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 215:3; ISSN ASJOA
Country of Publication:
United States
Language:
English