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      ExoMol molecular line lists - XIV: The rotation-vibration spectrum of hot SO\(_2\)

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          Abstract

          Sulphur dioxide is well-known in the atmospheres of planets and satellites, where its presence is often associated with volcanism, and in circumstellar envelopes of young and evolved stars as well as the interstellar medium. This work presents a line list of 1.3 billion \(^{32}\)S\(^{16}\)O\(_2\) vibration-rotation transitions computed using an empirically-adjusted potential energy surface and an ab initio dipole moment surface. The list gives complete coverage up to 8000 cm\(^{-1}\) (wavelengths longer than 1.25 \(\mu\)m) for temperatures below 2000 K. Infrared absorption cross sections are recorded at 300 and 500 C are used to validated the resulting ExoAmes line list. The line list is made available in electronic form as supplementary data to this article and at www.exomol.com.

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          Author and article information

          Journal
          2016-03-13
          Article
          10.1093/mnras/stw849
          1603.04065
          2a5dff4f-ec4d-409b-b70a-0be60fa2920a

          http://arxiv.org/licenses/nonexclusive-distrib/1.0/

          History
          Custom metadata
          MNRAS, 459, 3890-3899 (2016)
          Submitted to MNRAS
          astro-ph.EP astro-ph.SR

          Planetary astrophysics,Solar & Stellar astrophysics
          Planetary astrophysics, Solar & Stellar astrophysics

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