Neutral hydrogen at high redshift: probing structure formation

Details Neutral hydrogen at high redshift: probing structure formation Neutral hydrogen at high redshift: probing structure formation

1998-01-23

arxiv.org/abs/astro-ph/9801223v1

Astronomy and Astrophysics

Astrophysics

8 pages LaTeX, uses paspconf.sty and epsf.sty. To appear in "Highly Redshifted Radio Lines", eds. C. Carilli, S. Radford, K. M

Scientific paper

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.

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