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http://hdl.handle.net/2289/859
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DC Field | Value | Language |
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dc.contributor.author | Sethi, S.K. | - |
dc.date.accessioned | 2005-12-26T08:49:40Z | - |
dc.date.available | 2005-12-26T08:49:40Z | - |
dc.date.issued | 2005-04-10 | - |
dc.identifier.citation | Current Science, 2005, Vol. 88, p1117-1124. | en |
dc.identifier.issn | 0011-3891 | - |
dc.identifier.uri | http://hdl.handle.net/2289/859 | - |
dc.description.abstract | Recent years have seen major advances in understand-ing the state of the intergalactic medium (IGM) at high redshift. Some aspects of this understanding are reviewed here. In particular, we discuss: (1) Different probes of IGM like Gunn–Peterson test, CMBR anisotropies, and neutral hydrogen emission from reionization, and (2) some models of reionization of the universe. | en |
dc.format.extent | 166474 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Indian Academy of Sciences, Bangalore, India. | en |
dc.rights | Indian Academy of Sciences, Bangalore, India. | en |
dc.title | High redshift intergalactic medium: Probes and physical models | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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2005 CS V88 p1117.pdf | 8p. | 162.57 kB | Adobe PDF | View/Open |
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