Journalartikel

Jahr der Veröffentlichung: 2014

Seiten: 1828-1835

Zeitschrift: Monthly Notices of the Royal Astronomical Society

Bandnummer: 437

Heftnummer: 2

ISSN: 0035-8711

eISSN: 1365-2966

Open Access Status: Green

DOI Link: https://doi.org/10.1093/mnras/stt2011

Verlag: Oxford University Press

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.

Harvard-Zitierstil: Barber, R., Strange, J., Hill, C., Polyansky, O., Mellau, G., Yurchenko, S., et al. (2014) ExoMol line lists - III. An improved hot rotation-vibration line list for HCN and HNC, Monthly Notices of the Royal Astronomical Society, 437(2), pp. 1828-1835. https://doi.org/10.1093/mnras/stt2011

APA-Zitierstil: Barber, R., Strange, J., Hill, C., Polyansky, O., Mellau, G., Yurchenko, S., & 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. 437(2), 1828-1835. https://doi.org/10.1093/mnras/stt2011