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Properties of brightest cluster galaxies

Research datakeyboard_double_arrow_right Dataset 01 Jan 2023Publisher:Centre de Donnees Strasbourg (CDS)Funded by:NSF | Pan-STARRS1: Operations; ..., EC | LACEGAL
Authors: De Propris, R.; West, M.J.; Andrade-Santos, F.; Ragone-Figueroa, C.; Rasia, E.; Forman, W.; Jones, C.; +5 Authors

doi: 10.26093/cds/vizier.75000310

Properties of brightest cluster galaxies

Abstract

VizieR online Data Catalogue associated with article published in journal Monthly Notices of the Royal Astronomical Society with title ' Brightest cluster galaxies: the centre can(not?) hold.' (bibcode: 2021MNRAS.500..310D)

Keywords

galactic and extragalactic astronomy, Astrophysics and Astronomy, Physics, Galaxy clusters, Redshifted, Galactic and extragalactic Astronomy, Galaxies, X-ray sources, visible astronomy, Cosmology, Optical astronomy, observational astronomy, galaxy kinematics, Observational Astronomy, x ray sources, galaxies, galaxy clusters, redshifted, Natural Sciences, cosmology, Galaxy kinematics

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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!
0
Average
Average
Average
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