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Molecular hydrogen formation on dust grains in the high-redshift universe
S. Cazaux
*
, M. Spaans
*
Corresponding author for this work
Research output
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Contribution to journal
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Article
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Scientific
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peer-review
60
Citations (Scopus)
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Dive into the research topics of 'Molecular hydrogen formation on dust grains in the high-redshift universe'. Together they form a unique fingerprint.
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INIS
red shift
100%
hydrogen
100%
universe
100%
dusts
100%
gases
40%
abundance
30%
surfaces
20%
electrons
10%
kinetics
10%
values
10%
stars
10%
feedback
10%
range
10%
density
10%
far ultraviolet radiation
10%
radiations
10%
Physics
Galactic Radiation
10%