Role of different isomers of the H2CN+ ion in the formation of interstellar HCN and HNC

[1]  H. Schaefer,et al.  Formulation of the direct configuration interaction method for triplet spin states. Applications to glyoxal , 1978 .

[2]  R. Brown Deuterium enrichment in interstellar HCN and HNC , 1977, Nature.

[3]  M. McEwan,et al.  Laboratory investigation of some ion–molecule reactions related to cyanide chemistry in dense interstellar clouds , 1977 .

[4]  R. Taft,et al.  Gas phase basicities and relative proton affinities of compounds between water and ammonia from pulsed ion cyclotron resonance thermal equilibriums measurements , 1977 .

[5]  N. Adams,et al.  Reactions of CH + n IONS with ammonia at 300 K , 1977 .

[6]  F. C. Felisenfeld Ion Reactions with Atomic Oxygen and Atomic Nitrogen of Astrophysical Importance , 1976 .

[7]  P. K. Pearson,et al.  Some properties of H$sub 2$CN$sup +$: A potentially important interstellar species , 1974 .

[8]  Eric Herbst,et al.  The formation and depletion of molecules in dense interstellar clouds , 1973 .

[9]  William D. Watson,et al.  The Rate of Formation of Interstellar Molecules by Ion-Molecule Reactions , 1973 .

[10]  H. Schaefer The electronic structure of atoms and molecules : a survey of rigorous quantum mechanical results , 1972 .

[11]  T. H. Dunning Gaussian Basis Functions for Use in Molecular Calculations. III. Contraction of (10s6p) Atomic Basis Sets for the First‐Row Atoms , 1970 .

[12]  J. Bearden,et al.  Atomic energy levels , 1965 .

[13]  Edward Teller,et al.  Electronic Spectra of Polyatomic Molecules , 1941 .