High redshift intergalactic medium:  Probes and physical models

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/859

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DC Field	Value	Language
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)

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