The broad relationship between X-ray and radio luminosities for AGN
Abstract
AGN activity is often revealed by strong X-ray and radio emission, even when the AGN is obscured at other wavelengths. Some AGN have been observed to be radio bright but X-ray faint, others X-ray bright but radio faint, as well as bright or faint/unobserved in both X-ray and radio. What determines whether the AGN will be X-ray or radio bright? Is it due to one mechanism that determines both, or two mechanisms in isolation, or even some mixture of the two?
Fields of Study & Subjects
Galaxies: Formation
Evolution
Phenomena
Astrophysical Phenomena and Observations
Astrophysics and Cosmic Phenomena
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 27 February 2026
- Language
- EN