Fine-scale anisotropy of cosmic gamma-ray background to identify the underlying generation process

Details Fine-scale anisotropy of cosmic gamma-ray background to identify the underlying generation process Fine-scale anisotropy of cosmic gamma-ray background to identify the underlying generation process

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...348...33c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 348, Jan. 1, 1990, p. 33-37. Research supported by the University of Califo

Mathematics

Logic

6

Active Galactic Nuclei, Anisotropic Media, Cosmology, Gamma Rays, Quasars, Relic Radiation, Seyfert Galaxies, Galactic Evolution, High Resolution, Milky Way Galaxy, Monte Carlo Method, Red Shift

Scientific paper

The study of the intrinsic anisotropies of the extragalactic gamma-ray background is of cosmological importance. As the first step to investigate the anisotropies, new evolutionary results of the active galaxies are introduced and the fine-scale anisotropy is calculated because of the possible contribution from the AGN model. By use of Monte Carlo simulations, the fine-scale fluctuation patterns are discussed and it is proposed that these patterns or anisotropies form a unique test for the AGN generation mechanism.

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