Intracluster light in the core of z ∼ 2 galaxy proto-clusters

Intracluster light is thought to originate from stars that were ripped away from their parent galaxies by gravitational tides and galaxy interactions during the build up of the cluster. The stars from such interactions will accumulate over time, so semi-analytic models suggest that the abundance of...

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Main Authors: Werner, Stephane (Author) , Hatch, N A (Author) , Matharu, J (Author) , Gonzalez, A H (Author) , Bahé, Y M (Author) , Mei, S (Author) , Noirot, G (Author) , Wylezalek, Dominika (Author)
Format: Article (Journal)
Language:English
Published: July 2023
In: Monthly notices of the Royal Astronomical Society
Year: 2023, Volume: 523, Issue: 1, Pages: 91-104
ISSN:1365-2966
DOI:10.1093/mnras/stad1410
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stad1410
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Author Notes:S.V. Werner, N.A. Hatch, J. Matharu, A.H. Gonzalez, Y.M. Bahé, S. Mei, G. Noirot and D. Wylezalek
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Faint (C i)(1-0) emission in z [approximately] 3.5 radio galaxies by Kolwa, Sthabile (Author) , De Breuck, C (Author) , Vernet, J (Author) , Wylezalek, Dominika (Author) , Wang, Wuji (Author) , Popping, G (Author) , Man, A W S (Author) , Harrison, C M (Author) , Andreani, P (Author) ,


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