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Evolution of the gaseous content of the universeResults of a new spectroscopic survey for damped Ly-alpha absorption systems conducted at ultraviolet wavelengths are combined with those of previous surveys conducted at optical wavelengths in order to examine the evolution of the gaseous content of the universe at z between 0 and 3.5. Implications for scenarios of galaxy formation and evolution are discussed.
Document ID
19940034427
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/133283
Authors
Lanzetta, Kenneth M. (California Univ. La Jolla, United States)
Date Acquired
August 16, 2013
Publication Date
September 1, 1993
Publication Information
Publication: Astronomical Society of the Pacific, Publications
Volume: 105
Issue: 691
ISSN: 0004-6280
Subject Category
Astrophysics
Accession Number
94A11082
Funding Number(s)
CONTRACT_GRANT: NAS5-26555
Distribution Limits
Public
Copyright
Other

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