High redshift intergalactic medium: Probes and physical models
| dc.contributor.author | Sethi, Shiv | |
| dc.date.accessioned | 2005-12-26T08:49:40Z | |
| dc.date.available | 2005-12-26T08:49:40Z | |
| dc.date.issued | 2005-04-10 | |
| 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.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.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 |