Hostname: page-component-cd9895bd7-jn8rn Total loading time: 0 Render date: 2024-12-28T02:36:57.425Z Has data issue: false hasContentIssue false
  • English
  • Français

Damped Lyman-α Systems at Intermediate Redshifts

Published online by Cambridge University Press:  21 April 2007

E. Emsellem ,
H. Wozniak ,
G. Massacrier ,
J.-F. Gonzalez ,
J. Devriendt ,
N. Champavert  and
C. Péroux
C. Péroux*
Affiliation:
European Southern Observatory, Germany
Get access

Abstract

A complementary method to the emission selection of high-redshiftgalaxies consists in the observation of absorbers along the line ofsight toward a background quasar. This selection technique has aconstant sensitivity at all redshifts up to z = 6 (i.e. no redshiftdesert) and allow to select all types of galaxies regardless of theirluminosity or star formation rate. The highest column densityabsorbers, the Damped Lyman-α (DLAs) systems, in particular,can be used to determine the cosmic evolution of HI gas in theUniverse, ΩHI, and the global metallicity in the gasphase. Since stars are known to form from HI gas, ΩHIprovides an indirect tracer of the history of starformation. Recent results from several parallel VLT programmes aimingat determining the cosmological evolution of the metallicity in theneutral gas phase are presented.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 24: CRAL-2006. Chemodynamics: From First Stars to Local Galaxies , 2007 , pp. 203 - 208
Copyright
© EAS, EDP Sciences, 2007

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)