Numerical analysis of nanograin collision by classical molecular dynamics [electronic resource]
Interstellar dust grains [1] comprise only 1% of the mass in the molecular clouds of galaxies and yet catalyze the formation of many gas phase molecules, in particular H2 [2], which allows for the cooling and collapse of these clouds and the formation of stars and planets. High-energy radiation and...
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Online Access (via OSTI) |
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| Format: | Government Document Electronic eBook |
| Language: | English |
| Published: |
Washington, D.C. : Oak Ridge, Tenn. :
United States. Department of Energy. ; distributed by the Office of Scientific and Technical Information, U.S. Department of Energy,
2007.
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| Subjects: |
Internet
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| Call Number: |
E 1.99:ucrl-proc-234441
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| E 1.99:ucrl-proc-234441 | Available |