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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2829
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dc.contributor.authorNarasimha, D-
dc.date.accessioned2008-07-22T12:06:33Z-
dc.date.available2008-07-22T12:06:33Z-
dc.date.issued2002-09-
dc.identifier.citationBASI, Vol. 30, No. 3, pp. 723 - 728en
dc.identifier.urihttp://hdl.handle.net/2248/2829-
dc.description.abstractThe time delay between the multiple images in gravitational lens systems is affected by large scale mass distribution in the lens, even though it might not have observable effects on the macro images. Inhomogeneity at very small scale will not directly affect the time delay but will influence the models of mass distribution in the lens galaxy. How this degeneracy can be eliminated is described. A method to determine time delay based on smoothed cubic splines is explained. The value of the Hubble Constant, inferred from the time delay in 5 well-constrained lens systems is 56 ± 8 kIn S-1 Mpc-1•en
dc.format.extent247611 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectCosmologyen
dc.subjectCosmological Parametersen
dc.subjectHubble Constanten
dc.subjectGravitational-Lensing - Time Delayen
dc.titleTime delay in gravitational lens systems and cosmological parametersen
dc.typeArticleen
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