4.7 Article

ExoMol line lists - III. An improved hot rotation-vibration line list for HCN and HNC

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 437, Issue 2, Pages 1828-1835

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stt2011

Keywords

molecular data; opacity; astronomical data bases: miscellaneous; planets and satellites: atmospheres; stars: low-mass

Funding

  1. ERC [267219]
  2. Nuffield Foundation
  3. EPSRC [EP/J003921/1] Funding Source: UKRI
  4. STFC [ST/J001511/1, ST/I001050/1] Funding Source: UKRI
  5. Engineering and Physical Sciences Research Council [EP/J003921/1] Funding Source: researchfish
  6. Science and Technology Facilities Council [ST/J001511/1, ST/I001050/1] Funding Source: researchfish

Ask authors/readers for more resources

A revised rotation-vibration line list for the combined hydrogen cyanide (HCN)/hydrogen isocyanide (HNC) system is presented. The line list uses ab initio transition intensities calculated previously and extensive data sets of recently measured experimental energy levels. The resulting line list has significantly more accurate wavelengths than previous ones for these systems. An improved value for the separation between HCN and HNC is adopted, leading to an approximately 25 per cent lower predicted thermal population of HNC as a function of temperature in the key 2000 to 3000 K region. Temperature-dependent partition functions and equilibrium constants are presented. The line lists are validated by comparison with laboratory spectra and are presented in full as supplementary data to the article and at www.exomol.com.

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