The Balance of Dark and Luminous Mass in Rotating Galaxies

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dc.contributor.authorMcGaugh, Stacy S.
dc.date.accessioned2009-01-07T17:57:13Z
dc.date.available2009-01-07T17:57:13Z
dc.date.issued2005
dc.description.abstractbaryons to the total rotation velocity increases, the contribution of the dark matter decreases by a compensating amount. This poses a fine-tuning problem for CDM galaxy formation models, and may point to new physics for dark matter particles or even a modification of gravity.en
dc.format.extent285691 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationThe Balance of Dark and Luminous Mass in Rotating Galaxies. McGaugh, S.S. 2005, Phys. Rev. Lett., 95, 171302en
dc.identifier.urihttp://hdl.handle.net/1903/8709
dc.language.isoen_USen
dc.publisherCopyright 2005 The American Physical Societyen
dc.relation.isAvailableAtAstronomyen_us
dc.relation.isAvailableAtCollege of Computer, Mathematical & Physical Sciencesen_us
dc.relation.isAvailableAtDigital Repository at the University of Marylanden_us
dc.relation.isAvailableAtUniversity of Maryland (College Park, MD)en_us
dc.rights.licensePublisher version: http://prola.aps.org/abstract/PRL/v95/i17/e171302
dc.subjectdark massen
dc.subjectbaryonic massen
dc.subjectgalaxiesen
dc.titleThe Balance of Dark and Luminous Mass in Rotating Galaxiesen
dc.typeArticleen

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