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The dark matter haloes of massive, relaxed galaxy clusters observed with Chandra

โœ Scribed by R. W. Schmidt; S. W. Allen

Book ID
110842038
Publisher
John Wiley and Sons
Year
2007
Tongue
English
Weight
584 KB
Volume
379
Category
Article
ISSN
0035-8711

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We compare the measurement of the gravitational mass of 38 high-redshift galaxy clusters observed by Chandra using Modified Newtonian Dynamics (MOND) and standard Newtonian gravity. Our analysis confirms earlier findings that MOND cannot explain the difference between the baryonic mass and the total