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Inferring the dark matter splashback radius from cluster gas and observable profiles in the FLAMINGO simulations (2024)

First Author: Towler I

Attributed to: DiRAC-2.5 DC - Operations 2017-2020 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stae654

Publication URI: http://dx.doi.org/10.1093/mnras/stae654

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 3