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

Galaxy clusters contain vast amount of dark matter and baryonic matter. Here the authors show the observational detection of the anti-correlation of gas mass and stellar mass observables in the most massive galaxy clusters, indicating such clusters retain close to the cosmic mix of baryons and dark...

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Main Authors: Arya Farahi, Sarah L. Mulroy, August E. Evrard, Graham P. Smith, Alexis Finoguenov, Hervé Bourdin, John E. Carlstrom, Chris P. Haines, Daniel P. Marrone, Rossella Martino, Pasquale Mazzotta, Christine O’Donnell, Nobuhiro Okabe
Format: Article
Language:English
Published: Nature Publishing Group 2019-07-01
Series:Nature Communications
Online Access:https://doi.org/10.1038/s41467-019-10471-y
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spelling doaj-3eb77918f5484227839b9e9b5f7e48082021-05-11T12:39:26ZengNature Publishing GroupNature Communications2041-17232019-07-011011710.1038/s41467-019-10471-yDetection of anti-correlation of hot and cold baryons in galaxy clustersArya Farahi0Sarah L. Mulroy1August E. Evrard2Graham P. Smith3Alexis Finoguenov4Hervé Bourdin5John E. Carlstrom6Chris P. Haines7Daniel P. Marrone8Rossella Martino9Pasquale Mazzotta10Christine O’Donnell11Nobuhiro Okabe12Department of Physics, University of MichiganSchool of Physics and Astronomy, University of BirminghamDepartment of Physics, University of MichiganSchool of Physics and Astronomy, University of BirminghamDepartment of Physics, University of HelsinkiHarvard Smithsonian Centre for AstrophysicsKavli Institute for Cosmological Physics, Department of Astronomy and Astrophysics, University of ChicagoINAF - Osservatorio Astronomico di BreraSteward Observatory, University of ArizonaDipartimento di Fisica, Università degli Studi di Roma “Tor Vergata”Harvard Smithsonian Centre for AstrophysicsSteward Observatory, University of ArizonaDepartment of Physical Science, Hiroshima UniversityGalaxy clusters contain vast amount of dark matter and baryonic matter. Here the authors show the observational detection of the anti-correlation of gas mass and stellar mass observables in the most massive galaxy clusters, indicating such clusters retain close to the cosmic mix of baryons and dark matter.https://doi.org/10.1038/s41467-019-10471-y
collection DOAJ
language English
format Article
sources DOAJ
author Arya Farahi
Sarah L. Mulroy
August E. Evrard
Graham P. Smith
Alexis Finoguenov
Hervé Bourdin
John E. Carlstrom
Chris P. Haines
Daniel P. Marrone
Rossella Martino
Pasquale Mazzotta
Christine O’Donnell
Nobuhiro Okabe
spellingShingle Arya Farahi
Sarah L. Mulroy
August E. Evrard
Graham P. Smith
Alexis Finoguenov
Hervé Bourdin
John E. Carlstrom
Chris P. Haines
Daniel P. Marrone
Rossella Martino
Pasquale Mazzotta
Christine O’Donnell
Nobuhiro Okabe
Detection of anti-correlation of hot and cold baryons in galaxy clusters
Nature Communications
author_facet Arya Farahi
Sarah L. Mulroy
August E. Evrard
Graham P. Smith
Alexis Finoguenov
Hervé Bourdin
John E. Carlstrom
Chris P. Haines
Daniel P. Marrone
Rossella Martino
Pasquale Mazzotta
Christine O’Donnell
Nobuhiro Okabe
author_sort Arya Farahi
title Detection of anti-correlation of hot and cold baryons in galaxy clusters
title_short Detection of anti-correlation of hot and cold baryons in galaxy clusters
title_full Detection of anti-correlation of hot and cold baryons in galaxy clusters
title_fullStr Detection of anti-correlation of hot and cold baryons in galaxy clusters
title_full_unstemmed Detection of anti-correlation of hot and cold baryons in galaxy clusters
title_sort detection of anti-correlation of hot and cold baryons in galaxy clusters
publisher Nature Publishing Group
series Nature Communications
issn 2041-1723
publishDate 2019-07-01
description Galaxy clusters contain vast amount of dark matter and baryonic matter. Here the authors show the observational detection of the anti-correlation of gas mass and stellar mass observables in the most massive galaxy clusters, indicating such clusters retain close to the cosmic mix of baryons and dark matter.
url https://doi.org/10.1038/s41467-019-10471-y
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