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Cited by 323

The DOI matches its Crossref record; 23 of the 23 references it cites were found in a registry or an index.

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

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Barber, R. J., Strange, J. K., Hill, C., Polyansky, O. L., Mellau, G. Ch., Yurchenko, S. N., Tennyson, Jonathan·2014·Monthly Notices of the Royal Astronomical Society

Abstract

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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Metadata

Authors
Barber, R. J., Strange, J. K., Hill, C., Polyansky, O. L., Mellau, G. C., Yurchenko, S. N., & Tennyson, J.
Venue
Monthly Notices of the Royal Astronomical Society
Published
2013-11-14
Volume
437
Issue
2
Pages
1828-1835
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W2088586328
Cited by
323
References
23
FWCI
3.43
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: ExoMol line lists – III. An improved hot rotation-vibration line list for HCN and HNC. https://app.cochat.ai/papers/10.1093/mnras/stt2011
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Barber, R. J., Strange, J. K., Hill, C., Polyansky, O. L., Mellau, G. C., Yurchenko, S. N., & Tennyson, J. (2014). ExoMol line lists – III. An improved hot rotation-vibration line list for HCN and HNC. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/stt2011

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