Molecule formation and infrared emission in fast interstellar shocks. II - Dissociation speeds for interstellar shock waves

Details Molecule formation and infrared emission in fast interstellar shocks. II - Dissociation speeds for interstellar shock waves Molecule formation and infrared emission in fast interstellar shocks. II - Dissociation speeds for interstellar shock waves

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...241l..47h&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 241, Oct. 1, 1980, p. L47-L50.

Astronomy and Astrophysics

Astronomy

70

Emission Spectra, Infrared Astronomy, Interstellar Matter, Molecular Clouds, Shock Waves, Hydrogen Atoms, Interstellar Chemistry, Particle Collisions, Transition Probabilities, Vibrational Spectra

Scientific paper

The postshock destruction of molecules is examined, including the processes of (1) collisions with neutral hydrogen atoms and molecules, (2) electronic collisions, and (3) neutral chemical reactions with atoms, particularly atomic hydrogen. By using conservative estimates of collisional dissociation rates from individual vibrational states, it is found that process (1) leads to the destruction of molecular hydrogen behind shocks with speeds equal to or greater than 25 km/s if the preshock molecular gas has hydrogen nucleus densities of equal to or greater than 10 to the 4th/cu cm. At lower densities (100 per cu cm), destruction occurs for shock speeds equal to or greater than 50 km/s and process (2) dominates. Dissociation of molecules such as CO, H2O, and O2 follows the destruction of H2, as the resultant hydrogen atoms chemically dissociate the metal atoms from their bonds (process 3) in the hot postshock gas. These results demonstrate that many of the observed high-speed interstellar molecules, if shock accelerated, must have dissociated and reformed in the postshock gas.

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