Interpreting radiative efficiency in radio-loud AGNs

M. J. Hardcastle

doi:10.1038/s41550-018-0424-1

Interpreting radiative efficiency in radio-loud AGNs

M. J. Hardcastle

Research output: Contribution to journal › Review article

42 Citations (Scopus)

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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.

Original language	English
Pages (from-to)	273-274
Number of pages	2
Journal	Nature Astronomy
Volume	2
Issue number	4
Early online date	5 Apr 2018
DOIs	https://doi.org/10.1038/s41550-018-0424-1
Publication status	E-pub ahead of print - 5 Apr 2018

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1804.04043v1-csAccepted author manuscript, 275 KB

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title = "Interpreting radiative efficiency in radio-loud AGNs",

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.",

author = "Hardcastle, \{M. J.\}",

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

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AU - Hardcastle, M. J.

N1 - Author submitted version of unrefereed Nature Astronomy comment. Version in journal format available at https://rdcu.be/KH6W

PY - 2018/4/5

Y1 - 2018/4/5

N2 - 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.

AB - 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.

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U2 - 10.1038/s41550-018-0424-1

DO - 10.1038/s41550-018-0424-1

M3 - Review article

SN - 2397-3366

VL - 2

SP - 273

EP - 274

JO - Nature Astronomy

JF - Nature Astronomy

IS - 4

ER -

Interpreting radiative efficiency in radio-loud AGNs

Abstract

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