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Triaxiality in galaxy clusters: mass versus potential reconstructions

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Context. Accounting for the triaxial shapes of galaxy clusters will become important in the context of upcoming cosmological surveys. This will provide a challenge given that the density distribution of gas cannot be described by simple geometrical models without loss of information.Aims. We investi...

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Main Authors: Stapelberg, Sebastian (Author) , Tchernin, Céline (Author) , Hug, Damaris (Author) , Lau, E. T. (Author) , Bartelmann, Matthias (Author)
Format: Article (Journal)
Language:English
Published: 04 July 2022
In: Astronomy and astrophysics
Year: 2022, Volume: 663, Pages: 1-16
ISSN:1432-0746
DOI:10.1051/0004-6361/202040238
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1051/0004-6361/202040238
Verlag, lizenzpflichtig, Volltext: https://www.aanda.org/articles/aa/abs/2022/07/aa40238-20/aa40238-20.html
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Author Notes:S. Stapelberg, C. Tchernin, D. Hug, E.T. Lau, and M. Bartelmann
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Triaxiality in galaxy clusters: mass versus potential reconstructions by Stapelberg, Sebastian (Author) , Tchernin, Céline (Author) , Hug, Damaris (Author) , Lau, Erwin T. (Author) , Bartelmann, Matthias (Author) ,


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