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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3249
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dc.contributor.authorMajumdar, S-
dc.contributor.authorSubrahmanyan, R-
dc.date.accessioned2008-08-22T10:22:38Z-
dc.date.available2008-08-22T10:22:38Z-
dc.date.issued1999-12-
dc.identifier.citationPramana, Vol. 53, No. 6, pp. 971 - 975en
dc.identifier.issn0304-4289-
dc.identifier.urihttp://hdl.handle.net/2248/3249-
dc.description.abstractFor cold dark matter models, images of temperature fluctuations in the cosmic microwave background (CMB), due to Sunyaev Zel'dovich (SZ) effect have been been simulated taking a cosmological distribution of clusters into account. All the models are normalised to the 4-year COBE data. The image statistics are compared with the ATCA limits on arcmin scale anisotropy. The comparison appears to favour low-Ω0 open universe models.en
dc.format.extent334453 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy Of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/1999Prama..53..971Men
dc.subjectCosmic microwave backgrounden
dc.subjectTemperature fluctuationsen
dc.titleConstraining cosmological parameters through Sunyaev-Zel'dovich surveysen
dc.typeArticleen
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