Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997mnras.288..286g&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 288, Issue 2, pp. 286-294.
Astronomy and Astrophysics
Astronomy
4
Line: Formation, Molecular Processes, Ism: Molecules, Infrared: Ism: Lines And Bands
Scientific paper
We investigate the fates and population densities of the vibrationally excited homonuclear diatomic molecules H_2/H^+_2, C_2/C^+_2 and O_2/O^+_2 in interstellar conditions using photochemical kinetic models. We find that the population distribution of vibrationally excited H^+_2 resembles the nascent distribution from the cosmic ray ionization of H_2 under several cloud conditions. We predict that the density of H^+_2(v) could exceed that of H_2(v) under certain cloud conditions. Based on this we present a synthetic spectrum of the quadrupole-allowed infrared emission from H^+_2(v). Our results for H_2(v) are in accord with those of previous workers. The vibrationally excited states of C_2 and O_2 show abundances on the order of 10^-4 of the ground state. We emphasize that these populations are controlled by reaction dynamics and photochemical kinetics, and do not resemble those of the local thermodynamic equilibrium (LTE). Preliminary models of the C^+_2(v) and O^+_2(v) chemistry show that the vibrational distributions will somewhat resemble the nascent distributions of the reactions which create them. Further experimental or theoretical studies of the dynamics of these reactions are necessary before quantitative predictions can be made.
Glinski Robert J.
Nuth Joseph Andrew III
Schulz Stefan A.
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