Abstract
We consider the emission of high-energy to very-high-energy gamma -rays in radio-quiet active Galactic nuclei (AGN) or the central regions of radio-loud AGN. We use our results to estimate the gamma -ray flux from the central regions of nearby AGN and then to calculate the contribution to the diffuse gamma -ray flux from unresolved AGN.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callMore From: Journal of Physics G: Nuclear and Particle Physics
Paper Title
Journal
Date
