Dissociation equilibrium constants of molecules of astrophysical interest

Details Dissociation equilibrium constants of molecules of astrophysical interest Dissociation equilibrium constants of molecules of astrophysical interest

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..96..205r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 96, no. 1, Oct. 1983, p. 205-212. Research supported by the Fundacao de Am

Astronomy and Astrophysics

Astrophysics

4

Astrophysics, Chemical Equilibrium, Cosmochemistry, Dissociation, Molecular Spectra, Diatomic Molecules, Polyatomic Molecules, Protostars, Stellar Envelopes, Temperature Dependence

Scientific paper

Dissociation equilibrium constants are computed for 53 molecules containing H, C, N, O, Mg, Si, S, and Fe in a range of temperatures of astrophysical interest. The results are obtained using recent molecular constants and are compared with previously published data. The equilibrium constants are approximated by an analytical expression and the fitting coefficients are supplied.

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