NASA NTRS · 20060038916
Molecular Hydrogen-Rich Interstellar Ice
Abstract
While molecular hydrogen is by far the most abundant gas phase molecule in interstellar dark clouds, the extreme volatility of H(sub 2) suggests that it has a relatively low abundance in grain volatile mantles, thought to be composed largely of amorphous water ice.
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Dissly, R., Allen, M., Anicich, V.. 1993-01-01. Molecular Hydrogen-Rich Interstellar Ice. https://ntrs.nasa.gov/citations/20060038916
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