Neutral hydrogen at high redshift: probing structure formation

J. S. Bagla

Neutral hydrogen at high redshift: probing structure formation

Astrophysics 2007-05-23 v1

Authors: J. S. Bagla

Abstract

Large inhomogeneities in neutral hydrogen in the universe can be detected at redshifts $z \leq 10$ using the redshifted 21cm line emission from atomic hydrogen. This paper reviews the expected evolution of neutral hydrogen and presents estimates for future surveys of HI at $z \approx 3$ . We also discuss the possibility of detecting neutral hydrogen at higher redshifts.

Keywords

hydrogen storage and hydrides atomic hydrogen and helium systems

Cite

@article{arxiv.astro-ph/9801223,
  title  = {Neutral hydrogen at high redshift: probing structure formation},
  author = {J. S. Bagla},
  journal= {arXiv preprint arXiv:astro-ph/9801223},
  year   = {2007}
}

Comments

8 pages LaTeX, uses paspconf.sty and epsf.sty. To appear in "Highly Redshifted Radio Lines", eds. C. Carilli, S. Radford, K. Menten, G. Langston, (PASP: San Francisco)

Neutral hydrogen at high redshift: probing structure formation

Abstract

Keywords

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