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The Baryon Content Of Galaxy Clusters - A Challenge To Cosmological Orthodoxy

dc.contributor.authorWhite, S. D. M. (Simon D. M.)en_US
dc.contributor.authorNavarro, Julio F.en_US
dc.contributor.authorEvrard, August E.en_US
dc.contributor.authorFrenk, C. S.en_US
dc.date.accessioned2009-06-01T17:27:47Z
dc.date.available2009-06-01T17:27:47Z
dc.date.issued1993-12-02en_US
dc.identifier.citationWhite, SDM; Navarro, JF; Evrard, AE; Frenk, CS. (1993) "The Baryon Content Of Galaxy Clusters - A Challenge To Cosmological Orthodoxy." Nature 366(6454): 429-433. <http://hdl.handle.net/2027.42/62631>en_US
dc.identifier.issn0028-0836en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/62631
dc.description.abstractBaryonic matter constitutes a larger fraction of the total mass of rich galaxy clusters than is predicted by a combination of cosmic nucleosynthesis considerations (light-element formation during the Big Bang) and standard inflationary cosmology. This cannot be accounted for by gravitational and dissipative effects during cluster formation. Either the density of the Universe is less than that required for closure, or there is an error in the standard interpretation of element abundances.en_US
dc.format.extent626123 bytes
dc.format.extent2489 bytes
dc.format.mimetypeapplication/octet-stream
dc.format.mimetypetext/plain
dc.publisherMacmillan Magazines Ltd.en_US
dc.sourceNatureen_US
dc.titleThe Baryon Content Of Galaxy Clusters - A Challenge To Cosmological Orthodoxyen_US
dc.typeArticleen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumUNIV MICHIGAN,DEPT PHYS,ANN ARBOR,MI 48109en_US
dc.contributor.affiliationotherUNIV DURHAM,DEPT PHYS,DURHAM DH1 3LE,ENGLANDen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/62631/1/366429a0.pdf
dc.identifier.doihttp://dx.doi.org/10.1038/366429a0en_US
dc.identifier.sourceNatureen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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