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Cited by 282

The DOI matches its Crossref record; 19 of the 19 references it cites were found in a registry or an index.

On Black Hole Masses and Radio Loudness in Active Galactic Nuclei

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Laor, Ari·2000·The Astrophysical Journal

Abstract

The distribution of radio to optical fluxes in active galactic nuclei (AGNs) is bimodal. The physical origin for this bimodality is not understood. In this Letter I describe observational evidence, based on the Boroson & Green Palomar-Green quasar sample, that the radio loudness bimodality is strongly related to the black hole mass ( M BH ). Nearly all PG quasars with M BH > 10 9 M ☉ are radio-loud, while quasars with M BH < 3 × 10 8 M ☉ are practically all radio-quiet. This result is consistent with the dependence of quasar host galaxy morphology on radio loudness. There is no simple physical explanation for this result, but it may provide a clue as to how jets are formed near massive black holes. The radio loudness-black hole mass relationship suggests that the properties of various types of AGN may be largely set by three basic parameters: M BH , L / L Edd , and inclination angle.

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Metadata

Authors
Laor, A.
Venue
The Astrophysical Journal
Published
2000-11-10
Volume
543
Issue
2
Pages
L111-L114
ISSN
0004-637X (ISSN-L)
OpenAlex
W1558717895
Cited by
282
References
19
FWCI
14.08
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: On Black Hole Masses and Radio Loudness in Active Galactic Nuclei. https://app.cochat.ai/papers/10.1086/317280
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Laor, A. (2000). On Black Hole Masses and Radio Loudness in Active Galactic Nuclei. The Astrophysical Journal. https://doi.org/10.1086/317280

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