University of Hertfordshire

From the same journal

By the same authors

Interpreting radiative efficiency in radio-loud AGNs

Research output: Contribution to journalReview article

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Original languageEnglish
Number of pages2
Pages (from-to)273-274
JournalNature Astronomy
Journal publication date5 Apr 2018
Volume2
Issue4
Early online date5 Apr 2018
DOIs
Publication statusE-pub ahead of print - 5 Apr 2018

Abstract

Radiative efficiency in radio-loud active galactic nuclei is governed by the accretion rate onto the central black hole rather than directly by the type of accreted matter; while it correlates with real differences in host galaxies and environments, it does not provide unambiguous information about particular objects.

Notes

Author submitted version of unrefereed Nature Astronomy comment. Version in journal format available at https://rdcu.be/KH6W

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