Interpreting radiative efficiency in radio-loud AGN
Astrophysics of Galaxies
2018-04-12 v1 High Energy Astrophysical Phenomena
Abstract
Radiative efficiency in radio-loud AGN is governed by the scaled accretion rate on to the central black hole rather than directly by the type of accreted matter; while it correlates with real physical differences, it does not give us unambiguous information about particular objects.
Keywords
Cite
@article{arxiv.1804.04043,
title = {Interpreting radiative efficiency in radio-loud AGN},
author = {M. J. Hardcastle},
journal= {arXiv preprint arXiv:1804.04043},
year = {2018}
}
Comments
Author submitted version of unrefereed Nature Astronomy comment. Version in journal format available at https://rdcu.be/KH6W