@article {22760,
	title = {High-energy gamma radiation from extragalactic radio sources.},
	volume = {256},
	year = {1992},
	month = {1992/03/1},
	pages = {L27 - L30},
	abstract = {We propose that the important relationship between 3C 273 and 3C 279, the first two extragalactic sources detected at \&gt; 100 MeV energies, is their superluminal nature. In support of this conjecture, we propose a kinematic focusing mechanism, based on Compton scattering of accretion-disk photons by relativistic nonthermal electrons in the jet, that preferentially emits gamma rays in the superluminal direction.},
	keywords = {Accretion Disks, Compton Effect, Computational Astrophysics, Distribution Functions, Extragalactic Radio Sources, Gamma Ray Astronomy, Gamma Ray Observatory, Radio Emission, Relativistic Electron Beams, Space Radiation, Spaceborne Astronomy},
	isbn = {0004-6361},
	url = {https://ui.adsabs.harvard.edu/abs/1992A\&A...256L..27D},
	author = {Dermer, C. D. and Schlickeiser, R. and Mastichiadis, A.}
}
