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Galaxies and gamma-ray astronomy

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/157323· OSTI ID:5637071
Comparisons between the recently measured X-ray spectra of active galaxies, the intensity upper limits to the ..gamma..-ray emission above 35 MeV from the same objects obtained from data from SAS 2, and other ..gamma..-ray data are used to address the nature of the high-energy spectra of several types of active galaxies, their contribution to the measured diffuse ..gamma..-ray emission between 1 and 150 MeV, and constraints which may be placed on cosmological evolutionary factors. It is found that a substantial increase in slope of the photon energy spectrum must occur in the low-energy ..gamma..-ray region for Seyfert galaxies, BL Lac objects, and emission line galaxies. A spectral steepening is also seen for 3C 273 and Cen A, the only quasar and radio galaxy for which accurate X-ray spectra are presently available above 20 keV. A cosmological integration shows that Seyfert galaxies, BL Lac objects, and quasars may account for most of the 1--150 MeV diffuse background, even without significant evolution. Sharp emission line galaxies and radio galaxies made a much smaller contribution under the same assumptions. The observed isotropic ..gamma..-radiation limits the ..gamma..-ray evolution possible for Seyfert galaxies, BL Lac objects, and quasars. The high-latitude galactic radiation limits the ..gamma..-ray evolution of normal field galaxies. The integrated emission of normal field galaxies with evolution back to z=4 cannot exceed about 10 times the integrated emission assuming no evolution.
Research Organization:
NASA Goddard Space Flight Center
OSTI ID:
5637071
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 232:3; ISSN ASJOA
Country of Publication:
United States
Language:
English