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The Formation of Interstellar C2N Isomers in Circumstellar Envelopes of Carbon Stars: An Ab Initio Study

  • Authors: A. M. Mebel and R. I. Kaiser

Mebel & Kaiser 2002 The Astrophysical Journal 564 787.

  • Provider: AAS Journals

Caption: Fig. 2.

B3LYP/6‐311G** optimized geometries of intermediates, transition states, and products involved in the reaction of atomic carbon with hydrogen cyanide, together with their point groups and electronic wave functions. Important bond distances are given in angstroms, bond angles in degrees. Bold numbers show CCSD(T)/TZ2P optimized geometric parameters for the C2N isomers (Martin et al. 1994).

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