Infrared line emission by protogalaxies and protocluster pancakes

Details Infrared line emission by protogalaxies and protocluster pancakes Infrared line emission by protogalaxies and protocluster pancakes

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985azh....62..841s&link_type=abstract

(Astronomicheskii Zhurnal, vol. 62, Sept.-Oct. 1985, p. 841-846) Soviet Astronomy (ISSN 0038-5301), vol. 29, Sept.-Oct. 1985, p.

Astronomy and Astrophysics

Astronomy

2

Cosmic Gases, Galactic Clusters, Galactic Evolution, Hydrogen, Infrared Astronomy, H Ii Regions, Hydrogen Recombinations, Molecular Rotation, Stellar Radiation

Scientific paper

Calculations are performed to predict the properties of observable
infrared H I and H2 lines emitted by (1) the gas in protoclusters of
galaxies before the earliest stars and galaxies have formed, or (2) the
giant H II regions that would be excited by the star population in
individual primordial galaxies.

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