Evolution of Neutral Gas at High Redshift -- Implications for the Epoch of Galaxy Formation

Details Evolution of Neutral Gas at High Redshift -- Implications for the Epoch of Galaxy Formation Evolution of Neutral Gas at High Redshift -- Implications for the Epoch of Galaxy Formation

1996-08-22

arxiv.org/abs/astro-ph/9608147v1

Astronomy and Astrophysics

Astrophysics

To appear in MNRAS. Latex file (4 pages of text) plus 3 separate postscript figure files. Requires mn.sty. Postscript version

Scientific paper

Though observationally rare, damped Lya absorption systems dominate the mass density of neutral gas in the Universe. Eleven high redshift damped Lya systems covering 2.84 QSO Survey, extending these absorption system surveys to the highest redshifts currently possible. Combining our new data set with previous surveys we find that the cosmological mass density in neutral gas, omega_g, does not rise as steeply prior to z~2 as indicated by previous studies. There is evidence in the observed omega_g for a flattening at z~2 and a possible turnover at z~3. When combined with the decline at z>3.5 in number density per unit redshift of damped systems with column densities log N(HI)>21 atoms cm^-2, these results point to an epoch at z>3 prior to which the highest column density damped systems are still forming. We find that over the redshift range 2

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