Molecular Hydrogen in Pre-galactic Gas Clouds

Details Molecular Hydrogen in Pre-galactic Gas Clouds Molecular Hydrogen in Pre-galactic Gas Clouds

Dec 1967

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967natur.216..976s&link_type=abstract

Nature, Volume 216, Issue 5119, pp. 976-978 (1967).

Physics

97

Scientific paper

During the collapse of pre-galactic gas clouds through a density of
about 104 particles/cm3, hydrogen molecules are
produced and dominate the subsequent cooling.

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