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Interpreting radiative efficiency in radio-loud AGN
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Interpreting radiative efficiency in radio-loud AGN
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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.
Forward citations
Cited by 3 Pith papers
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