SIMBAD references

2003MNRAS.346.1103P - Mon. Not. R. Astron. Soc., 346, 1103-1115 (2003/December-3)

The evolution of ΩHIand the epoch of formation of damped Lyman α absorbers.

PEROUX C., McMAHON R.G., STORRIE-LOMBARDI L.J. and IRWIN M.J.

Abstract (from CDS):

We present a study of the evolution of the column density distribution, f (N, z), and total neutral hydrogen mass in high column density quasar absorbers using candidates from a recent high-redshift survey for damped Lyman α (DLA) and Lyman-limit system (LLS) absorbers. The observed number of LLS [N (HI) >1.6x1017 atom/cm2 ] is used to constrain f (N, z) below the classical DLA definition of 2x1020 atom/cm2. The evolution of the number density of LLS is consistent with our previous work but steeper than previously published work of other authors. At z 5, the number density of Lyman-limit systems per unit redshift is ∼5, implying that these systems are a major source of ultraviolet (UV) opacity in the high-redshift Universe. The joint LLS-DLA analysis shows unambiguously that f (N, z) deviates significantly from a single power law and that a Γ-law distribution of the form f (N, z) (f*/N*)(N/N*)–β exp(-N/N*) provides a better description of the observations. These results are used to determine the amount of neutral gas contained in DLAs and in systems with lower column density. Whilst in the redshift range 2-3.5, ∼90 per cent of the neutral HI mass is in DLAs, we find that at z > 3.5 this fraction drops to only 55 per cent and that the remaining `missing' mass fraction of the neutral gas lies in sub-DLAs with N (HI) 1019 -2x1020 atom/cm2. The characteristic column density, N*, changes from 1.6x1021 atom/cm2 at z < 3.5 to 2.9x1020 atom/cm2 at z > 3.5, supporting a picture where at z > 3.5, we are directly observing the formation of high column density neutral hydrogen DLA systems from lower column density units. Moreover, since current metallicity studies of DLA systems focus on the higher column density systems they may be giving a biased or incomplete view of global galactic chemical evolution at z > 3. After correcting the observed mass in HI for the `missing' neutral gas the comoving mass density now shows no evidence for a decrease above z 2.

Abstract Copyright: 2003 RAS

Journal keyword(s): galaxies: evolution - galaxies: formation - intergalactic medium - quasars: absorption lines - cosmology: observations

VizieR on-line data: <Available at CDS (J/MNRAS/346/1103): table1.dat refs.dat>

Simbad objects: 770

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2019.09.21-09:42:12

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