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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Autores principales:	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
Formato:	article
Lenguaje:	EN
Publicado:	Nature Portfolio 2019
Materias:	Science Q
Acceso en línea:	https://doaj.org/article/3eb77918f5484227839b9e9b5f7e4808
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spelling	oai:doaj.org-article:3eb77918f5484227839b9e9b5f7e48082021-12-02T15:36:06ZDetection of anti-correlation of hot and cold baryons in galaxy clusters10.1038/s41467-019-10471-y2041-1723https://doaj.org/article/3eb77918f5484227839b9e9b5f7e48082019-07-01T00:00:00Zhttps://doi.org/10.1038/s41467-019-10471-yhttps://doaj.org/toc/2041-1723Galaxy 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.Arya FarahiSarah L. MulroyAugust E. EvrardGraham P. SmithAlexis FinoguenovHervé BourdinJohn E. CarlstromChris P. HainesDaniel P. MarroneRossella MartinoPasquale MazzottaChristine O’DonnellNobuhiro OkabeNature PortfolioarticleScienceQENNature Communications, Vol 10, Iss 1, Pp 1-7 (2019)
institution	DOAJ
collection	DOAJ
language	EN
topic	Science Q
spellingShingle	Science Q 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
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.
format	article
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
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 Portfolio
publishDate	2019
url	https://doaj.org/article/3eb77918f5484227839b9e9b5f7e4808
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Detection of anti-correlation of hot and cold baryons in galaxy clusters

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