Interpreting radiative efficiency in radio-loud AGNs

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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.

Original languageEnglish
Pages (from-to)273-274
Number of pages2
JournalNature Astronomy
Issue number4
Early online date5 Apr 2018
Publication statusE-pub ahead of print - 5 Apr 2018


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