Figure 1 from Laboratory Detection of HOCN and Tentative Identification in Sgr B2

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Laboratory Detection of HOCN and Tentative Identification in Sgr B2

Authors: S. Brünken, C. A. Gottlieb, M. C. McCarthy, and P. Thaddeus

BRÜNKEN et al. 2009 The Astrophysical Journal 697 880.

Provider: AAS Journals

Caption: Figure 1.

Calculated equilibrium structures and relative energies of the CHNO isomers. Structures for HNCO, HOCN, and HCNO are from CCSD(T)/cc-pCV5Z calculations by ML; the structure of HONC (CCSD(T)/cc-pVQZ) and the relative energies are from SMAS.

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