Potential energy curves and dissociation energies of NbO, SiC, CP, PH(+), SiF(+), and NH(+)

Details Potential energy curves and dissociation energies of NbO, SiC, CP, PH(+), SiF(+), and NH(+) Potential energy curves and dissociation energies of NbO, SiC, CP, PH(+), SiF(+), and NH(+)

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.189...29r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 189, no. 1, March 1992, p. 29-38. Research supported by ISRO.

Astronomy and Astrophysics

Astrophysics

7

Dissociation, Interstellar Matter, Niobium Oxides, Phosphorus Compounds, Potential Energy, Silicon Carbides, Stellar Composition, Fluorides, Hydrides, Imides, Molecular Ions, Silicon Compounds

Scientific paper

The method by Rees (1947) is incorporated into the procedure by Vanderslice et al. (1960) to derive the potential-energy curves of the electronic ground states of six astrophysically significant molecules. The estimated dissociation energies are listed and used to compute D(0) values which agree with the previous values. The ionization potentials for PH, SiF, and NH are 10.12, 7.13, and 13.66 eV, respectively, and the dissociation energies of these molecules are also examined.

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