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Part of book or chapter of book . 2008 . Peer-reviewed
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“Radio–active” Brightest Cluster Galaxies

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Other literature type 11 Feb 2008 English Publisher:Springer Berlin Heidelberg
Authors: A. Linden der; P. N. Best; G. Kauffmann;

doi: 10.1007/978-3-540-73484-0_32

“Radio–active” Brightest Cluster Galaxies

Abstract

We present a sample of clusters drawn from the C4 cluster catalog of the Sloan Digital Sky Survey, where particular emphasis has been placed on the correct identification of the Brightest Cluster Galaxy (BCG) and the determination of the velocity dispersion within the virial radius. In this sample, we investigate the occurence of radio-AGN activity in the BCGs. We find that the radio-loud fraction is enhanced by a factor of up to 10, compared to galaxies of the same mass that are not BCGs.

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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!
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