On the Origin and Evolution of the Intra-Cluster Light: A Brief Review of the Most Recent Developments

Not all the light in galaxy groups and clusters comes from stars that are bound to galaxies. A significant fraction of it constitutes the so-called intracluster or diffuse light (ICL), a low surface brightness component of groups/clusters generally found in the surroundings of the brightest cluster...

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Main Author: Emanuele Contini
Format: Article
Language:English
Published: MDPI AG 2021-08-01
Series:Galaxies
Subjects:
Online Access:https://www.mdpi.com/2075-4434/9/3/60
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author Emanuele Contini
author_facet Emanuele Contini
author_sort Emanuele Contini
collection DOAJ
description Not all the light in galaxy groups and clusters comes from stars that are bound to galaxies. A significant fraction of it constitutes the so-called intracluster or diffuse light (ICL), a low surface brightness component of groups/clusters generally found in the surroundings of the brightest cluster galaxies and intermediate/massive satellites. In this review, I will describe the mechanisms responsible for its formation and evolution, considering the large contribution given to the topic in the last decades by both the theoretical and observational sides. Starting from the methods that are commonly used to isolate the ICL, I will address the remarkable problem given by its own definition, which still makes the comparisons among different studies not trivial, to conclude by giving an overview of the most recent works that take advantage of the ICL as a luminous tracer of the dark matter distribution in galaxy groups and clusters.
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spelling doaj.art-e8491d963b9a462e9a2bfa68843845a92023-11-22T13:10:42ZengMDPI AGGalaxies2075-44342021-08-01936010.3390/galaxies9030060On the Origin and Evolution of the Intra-Cluster Light: A Brief Review of the Most Recent DevelopmentsEmanuele Contini0School of Astronomy and Space Science, Nanjing University, Nanjing 210093, ChinaNot all the light in galaxy groups and clusters comes from stars that are bound to galaxies. A significant fraction of it constitutes the so-called intracluster or diffuse light (ICL), a low surface brightness component of groups/clusters generally found in the surroundings of the brightest cluster galaxies and intermediate/massive satellites. In this review, I will describe the mechanisms responsible for its formation and evolution, considering the large contribution given to the topic in the last decades by both the theoretical and observational sides. Starting from the methods that are commonly used to isolate the ICL, I will address the remarkable problem given by its own definition, which still makes the comparisons among different studies not trivial, to conclude by giving an overview of the most recent works that take advantage of the ICL as a luminous tracer of the dark matter distribution in galaxy groups and clusters.https://www.mdpi.com/2075-4434/9/3/60galaxy clustersgalaxy formationgalaxy evolution
spellingShingle Emanuele Contini
On the Origin and Evolution of the Intra-Cluster Light: A Brief Review of the Most Recent Developments
Galaxies
galaxy clusters
galaxy formation
galaxy evolution
title On the Origin and Evolution of the Intra-Cluster Light: A Brief Review of the Most Recent Developments
title_full On the Origin and Evolution of the Intra-Cluster Light: A Brief Review of the Most Recent Developments
title_fullStr On the Origin and Evolution of the Intra-Cluster Light: A Brief Review of the Most Recent Developments
title_full_unstemmed On the Origin and Evolution of the Intra-Cluster Light: A Brief Review of the Most Recent Developments
title_short On the Origin and Evolution of the Intra-Cluster Light: A Brief Review of the Most Recent Developments
title_sort on the origin and evolution of the intra cluster light a brief review of the most recent developments
topic galaxy clusters
galaxy formation
galaxy evolution
url https://www.mdpi.com/2075-4434/9/3/60
work_keys_str_mv AT emanuelecontini ontheoriginandevolutionoftheintraclusterlightabriefreviewofthemostrecentdevelopments