Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4095
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dc.contributor.authorNath, Biman B.-
dc.date.accessioned2011-08-11T07:45:18Z-
dc.date.available2011-08-11T07:45:18Z-
dc.date.issued2011-05-
dc.identifier.citationResonance, 2011, Vol.16, May, p428en
dc.identifier.issn0971-8044-
dc.identifier.issn0971-8044 (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/4095-
dc.descriptionOpen Accessen
dc.description.abstractSoon after the discovery of the cosmic background radiation, Zeldovich and Sunyaev proposed that hot gas in galaxy clusters should cast a faint shadow because of the interaction between energetic electrons and the radiation photons. Sunayev-Zeldovich effect is now routinely observed, and it has become an important tool for studying the history of the universe.en
dc.language.isoenen
dc.publisherIndian Academy of Sciences, Bangaloreen
dc.rights2011 Indian Academy of Sciences, Bangalore.en
dc.subjectCosmic background radiationen
dc.subjectcompton scatteringen
dc.titleSunyaev-Zeldovich effect: Shadows in the Cosmic Radiationen
dc.typeArticleen
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