University of Hertfordshire

From the same journal

By the same authors

Interpreting radiative efficiency in radio-loud AGN

Research output: ResearchArticle


  • 1804.04043v1

    Accepted author manuscript, 239 KB, PDF-document

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Original languageUndefined/Unknown
JournalNature Astronomy
Journal publication date11 Apr 2018
StatePublished - 11 Apr 2018


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.


Author submitted version of unrefereed Nature Astronomy comment. Version in journal format available at


ID: 13695675