Detection of anti-correlation of hot and cold baryons in galaxy clusters

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http://hdl.handle.net/10138/304649

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Farahi , A , Mulroy , S L , Evrard , A E , Smith , G P , Finoguenov , A , Bourdin , H , Carlstrom , J E , Haines , C P , Marrone , D P , Martino , R , Mazzotta , P , O'Donnell , C & Okabe , N 2019 , ' Detection of anti-correlation of hot and cold baryons in galaxy clusters ' , Nature Communications , vol. 10 , 2504 . https://doi.org/10.1038/s41467-019-10471-y

Title: Detection of anti-correlation of hot and cold baryons in galaxy clusters
Author: Farahi, Arya; Mulroy, Sarah L.; Evrard, August E.; Smith, Graham P.; Finoguenov, Alexis; Bourdin, Herve; Carlstrom, John E.; Haines, Chris P.; Marrone, Daniel P.; Martino, Rossella; Mazzotta, Pasquale; O'Donnell, Christine; Okabe, Nobuhiro
Contributor: University of Helsinki, Department of Physics
Date: 2019-07-02
Language: eng
Number of pages: 7
Belongs to series: Nature Communications
ISSN: 2041-1723
URI: http://hdl.handle.net/10138/304649
Abstract: The largest clusters of galaxies in the Universe contain vast amounts of dark matter, plus baryonic matter in two principal phases, a majority hot gas component and a minority cold stellar phase comprising stars, compact objects, and low-temperature gas. Hydrodynamic simulations indicate that the highest-mass systems retain the cosmic fraction of baryons, a natural consequence of which is anti-correlation between the masses of hot gas and stars within dark matter halos of fixed total mass. We report observational detection of this anti-correlation based on 4 elements of a 9 x 9-element covariance matrix for nine cluster properties, measured from multi-wavelength observations of 41 clusters from the Local Cluster Substructure Survey. These clusters were selected using explicit and quantitative selection rules that were then encoded in our hierarchical Bayesian model. Our detection of anti-correlation is consistent with predictions from contemporary hydrodynamic cosmological simulations that were not tuned to reproduce this signal.
Subject: SCALING RELATIONS
MASS
SIMULATIONS
SAMPLE
GAS
CHANDRA
LOCUSS
ASTROPHYSICS
COSMOLOGY
INFALL
115 Astronomy, Space science
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