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

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