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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2019-07-01
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Series: | Nature Communications |
Online Access: | https://doi.org/10.1038/s41467-019-10471-y |
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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 |
work_keys_str_mv |
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