Evolution in cluster cores since z~1

A large fraction of the stellar mass in galaxy clusters is thought to be contained in the diffuse low surface brightness intracluster light (ICL). Being bound to the gravitational potential of the cluster rather than any individual galaxy, the ICL contains much information about the evolution of its...

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Bibliographische Detailangaben

Veröffentlicht in:	arXiv.org 2012-11
Hauptverfasser:	Burke, Claire, Collins, Chris, Stott, John, Hilton, Matt
Format:	Artikel
Sprache:	eng
Schlagworte:	Galactic clusters Galactic evolution Galaxies Physics - Cosmology and Nongalactic Astrophysics Stars & galaxies Stellar mass Surface brightness
Online-Zugang:	Volltext
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