Intensity calculations of HCN molecules

Details Intensity calculations of HCN molecules Intensity calculations of HCN molecules

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aps..osf.e2003y&link_type=abstract

American Physical Society, Ohio Section of the APS Fall Meeting, October 13-14, 2006, abstract #E2.003

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Accurate spectroscopic data of HCN are required for many astronomical calculations and modeling. HCN molecules are present in the atmosphere of carbon stars and in galactic centers. Ro-vibrational energy levels and intensity calculations were carried out using the full coupled cluster model and radau coordinates. Accurate ab initio calculated potential energy surface^1 and dipole moment surface^2 were used for computation. The computed values were compared with Hitran^99.^

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