ON THE (NON)EVOLUTION OF H I GAS IN GALAXIES OVER COSMIC TIME
Authors:
- J. Xavier ProchaskaJ. Xavier Prochaska
- Arthur M. WolfeAWArthur M. Wolfe
- 24 April 2009
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 696 (2) , 1543-1547
Abstract
No abstract availableAll Related Versions
This publication has 36 references indexed in Scilit:
- z∼ 7–10 Galaxies in the HUDF and GOODS Fields: UV Luminosity FunctionsThe Astrophysical Journal, 2008
- The Fifth Data Release of the Sloan Digital Sky SurveyThe Astrophysical Journal Supplement Series, 2007
- Coincident, 100 kpc scale damped Lyα absorption towards a binary QSO: how large are galaxies at z ∼ 3?Monthly Notices of the Royal Astronomical Society, 2007
- Echelle Spectroscopy of a Gamma-Ray Burst Afterglow at z = 3.969: A New Probe of the Interstellar and Intergalactic Media in the Young UniverseThe Astrophysical Journal, 2005
- How do galaxies get their gas?Monthly Notices of the Royal Astronomical Society, 2005
- STAR FORMATION IN GALAXIES ALONG THE HUBBLE SEQUENCEAnnual Review of Astronomy and Astrophysics, 1998
- The formation of galactic discsMonthly Notices of the Royal Astronomical Society, 1998
- Damped Lyman-Alpha and Lyman-Limit Absorbers in the Cold Dark Matter ModelThe Astrophysical Journal, 1996
- The IUE Survey for Damped Lyman- alpha and Lyman-Limit Absorption Systems: Evolution of the Gaseous Content of the UniverseThe Astrophysical Journal, 1995
- The formation of the exponential disk in spiral galaxiesThe Astrophysical Journal, 1987