Interpreting radiative efficiency in radio-loud AGN
classification
🌌 astro-ph.GA
astro-ph.HE
keywords
efficiencyradiativeradio-loudaccretedaccretionblackcentralcorrelates
Add this Pith Number to your LaTeX paper
What is a Pith Number?\usepackage{pith}
\pithnumber{EDOYUIIK}
Prints a linked pith:EDOYUIIK badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.