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DC Field | Value | Language |
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dc.contributor.author | Nath, Biman B. | - |
dc.date.accessioned | 2011-08-11T07:45:18Z | - |
dc.date.available | 2011-08-11T07:45:18Z | - |
dc.date.issued | 2011-05 | - |
dc.identifier.citation | Resonance, 2011, Vol.16, May, p428 | en |
dc.identifier.issn | 0971-8044 | - |
dc.identifier.issn | 0971-8044 (Online) | - |
dc.identifier.uri | http://hdl.handle.net/2289/4095 | - |
dc.description | Open Access | en |
dc.description.abstract | Soon 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.iso | en | en |
dc.publisher | Indian Academy of Sciences, Bangalore | en |
dc.rights | 2011 Indian Academy of Sciences, Bangalore. | en |
dc.subject | Cosmic background radiation | en |
dc.subject | compton scattering | en |
dc.title | Sunyaev-Zeldovich effect: Shadows in the Cosmic Radiation | en |
dc.type | Article | en |
Appears in Collections: | Miscellaneous Publications |
Files in This Item:
File | Description | Size | Format | |
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2011_Resonance_May_p428.pdf | Open access | 1.01 MB | Adobe PDF | View/Open |
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