The formation of vibrationally excited hydrogen molecules on carbon surfaces.

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Molecular Data, Molecular Processes, Dust, Extinction, Ism: Molecules, Methods: Laboratory

Scientific paper

A novel technique for the measurement of the excitation of molecular hydrogen formed on surfaces has been applied to the study of H_2_ formation on carbon. The results show that on certain carbon surfaces H_2_ may form in vibrational levels as high as v=7, and that at a surface temperature of 90K between 2.6 and 7% of the molecules can be found in the v=1 level. This supports the proposal that a significant contribution to the population of vibrationally excited hydrogen in the interstellar medium comes from the formation of molecular hydrogen on carbonaceous interstellar grains.

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