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Molecular hydrogen formation on interstellar dust grains
S. A. Cohen
Astrophysical Sciences
PPPL Discovery Plasma Science
Plasma Physics Lab
Research output
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Contribution to journal
›
Article
›
peer-review
2
Scopus citations
Overview
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Dive into the research topics of 'Molecular hydrogen formation on interstellar dust grains'. Together they form a unique fingerprint.
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Engineering
Molecular Hydrogen
100%
Maximum Temperature
100%
Binding Energy
100%
Average Velocity
100%
Physisorption
100%
Dust Cloud
100%
Keyphrases
Molecular Hydrogen Formation
100%
Hydrogen Density
50%
Grain Temperature
50%
Gas-solid Systems
50%
Physics
Interstellar Dust
100%
Desorption
50%
Binding Energy
50%
Material Science
Density
100%
Desorption
100%
Chemical Engineering
Desorption
100%
Physisorption
100%