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Leiden University Scholarly Publications Repository
Article . 1988
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The Astrophysical Journal
Article . 1988 . Peer-reviewed
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The Astrophysical Journal
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https://dx.doi.org/10.1086/166...
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Jet precession in active galaxies

descriptionPublicationkeyboard_double_arrow_right Article 01 Nov 1988 Netherlands English Publisher:American Astronomical SocietyJournal:The Astrophysical Journal, volume 334, page 95 (issn: 0004-637X, eissn: 1538-4357, Copyright policy )
Authors: Roos, N.;

doi: 10.1086/166820

handle: 1887/6547

Jet precession in active galaxies

Abstract

The formation and evolution of massive binary black holes in galactic nuclei are studied with respect to the loss-cone filling model for the fueling of massive black holes in AGN during the final stage of galaxy mergers. A relation between the precession period of the jet and the fueling rate of the central hole has been obtained. It is shown that the characteristic time for position angle variation may be correlated with the level of central activity. 48 references.

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    		 40
    popularity
    This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
    		 Top 10%
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
40
Top 10%
Top 10%
Average
Green
gold
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