ExoMol molecular line lists - XXXVII. Spectra of acetylene

Katy L. Chubb, Jonathan Tennyson*, Sergei N. Yurchenko

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

65 Citations (Scopus)

Abstract

A new ro-vibrational line list for the ground electronic state of the main isotopologue of acetylene, (C2H2)-C-12, is computed as part of the ExoMol project. The aCeTY line list covers the transition wavenumbers up to 10 000 cm(-1) (lambda > 1 mu m), with lower and upper energy levels up to 12 000 and 22 000 cm(-1) considered, respectively. The calculations are performed up to a maximum value for the vibrational angular momentum, K-max = L-max = 16, and maximum rotational angular momentum, J = 99. Higher values of J were not within the specified wavenumber window. The aCeTY line list is considered to be complete up to 2200 K, making it suitable for use in characterizing high-temperature exoplanet or cool stellar atmospheres. Einstein-A coefficients, which can directly be used to calculate intensities at a particular temperature, are computed for 4.3 billion (4 347 381 911) transitions between 5 million (5 160803) energy levels. We make comparisons against other available data for (C2H2)-C-12, and demonstrate this to be the most complete line list available. The line list is available in electronic form from the online CDS and ExoMol data bases.

Original languageEnglish
Pages (from-to)1531-1545
Number of pages15
JournalMonthly Notices of the Royal Astronomical Society
Volume493
Issue number2
DOIs
Publication statusPublished - Apr 2020

Keywords

  • molecular data
  • planets and Satellites: atmospheres
  • stars: atmosphere
  • stars: carbon
  • ROTATION-VIBRATION SPECTRUM
  • DYNAMIC-MODEL ATMOSPHERES
  • NEAR-INFRARED SPECTRA
  • CARBON STARS
  • ABSORPTION-SPECTRUM
  • SPECTROSCOPIC DATA
  • AGB STARS
  • CHEMISTRY
  • METHANE
  • CM(-1)

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