Evolution of the gaseous content of the universe

Details Evolution of the gaseous content of the universe Evolution of the gaseous content of the universe

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pasp..105.1063l&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 105, no. 691, p. 1063-1069.

Astronomy and Astrophysics

Astronomy

10

Astronomical Spectroscopy, Galactic Evolution, Interstellar Gas, Lyman Alpha Radiation, Neutral Gases, Ultraviolet Radiation, Red Shift, Sky Surveys (Astronomy), Universe

Scientific paper

Results 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.

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