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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2980
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dc.contributor.authorSivaram, C-
dc.date.accessioned2008-08-04T10:20:13Z-
dc.date.available2008-08-04T10:20:13Z-
dc.date.issued1994-09-
dc.identifier.citationAstrophysics and Space Science, Vol. 219, No. 1, pp. 135 - 141en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/2980-
dc.description.abstractA possible connection between MOND (Modification of Newtonian Dynamics) proposed as an alternative hypothesis to dark matter in galaxies and clusters and a residual cosmological constant term dominating cosmological dynamics in a Omega = 1 universe is explored.en
dc.format.extent3894 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://www.springerlink.com/content/l2880650x54u2640/en
dc.subjectAstrodynamicsen
dc.subjectConstantsen
dc.subjectCosmologyen
dc.subjectDark Matteren
dc.subjectGalactic Clustersen
dc.subjectGalaxiesen
dc.subjectMissing Mass (Astrophysics)en
dc.subjectNewton Theoryen
dc.subjectUniverseen
dc.subjectFlux Densityen
dc.subjectGalactic Rotationen
dc.subjectPoisson Equationen
dc.subjectSpiral Galaxiesen
dc.subjectStellar Gravitationen
dc.subjectVacuumen
dc.titleMond, dark matter and the cosmological constanten
dc.typeArticleen
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