Molecular evolution in astrophysical environments.
Molecular formation and destruction processes are explored in rapidly evolving, non-equilibrium astrophysical environments. First, a semi-classical calculation is made for the rate coefficients of excited atom radiative association to form molecular hydrogen and of the process C⁺ + O → CO⁺ + hν. The...
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| Language: | en |
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The University of Arizona.
1989
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| Online Access: | http://hdl.handle.net/10150/184864 |