High Redshift Intergalactic Medium: Probes and Physical Models

Simple item page
dc.creatorSethi, Shiv K.
dc.date2004-11-02
dc.date.accessioned2026-07-07T02:15:38Z
dc.date.available2026-07-07T02:15:38Z
dc.descriptionRecent years have seen major advances in understanding 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.
dc.description20 pages, 8 figures, Invited article; to appear in Current Science (special section on Cosmology)
dc.identifierhttps://arxiv.org/abs/astro-ph/0411050
dc.identifierhttp://arxiv.org/abs/astro-ph/0411050
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8478
dc.subjectAstrophysics
dc.titleHigh Redshift Intergalactic Medium: Probes and Physical Models
dc.typetext

Files

Collections

arXiv