Shock-accelerated non-thermal electrons produce AGN radio synchrotron and X-ray IC emission whose scalings with accretion rate and black-hole mass recover observed radio-loudness trends and fundamental-plane slopes.
L., Bechtold, J., & Elvis, M
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A Shock-based Interpretation of Radio and X-ray Emission in Active Galactic Nuclei
Shock-accelerated non-thermal electrons produce AGN radio synchrotron and X-ray IC emission whose scalings with accretion rate and black-hole mass recover observed radio-loudness trends and fundamental-plane slopes.