ExoMol molecular line lists XX: a comprehensive line list for H$_3^+$
| Autor: | Oleg L. Polyansky, Alexander Alijah, Nikolai F. Zobov, Sergei N. Yurchenko, Aleksandra A. Kyuberis, Lorenzo Lodi, Jonathan Tennyson, Irina I. Mizus |
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| Rok vydání: | 2017 |
| Předmět: |
Gas giant
media_common.quotation_subject FOS: Physical sciences Astrophysics 01 natural sciences Planet Physics - Chemical Physics 0103 physical sciences 010306 general physics 010303 astronomy & astrophysics Astrophysics::Galaxy Astrophysics Solar and Stellar Astrophysics (astro-ph.SR) media_common Physics Earth and Planetary Astrophysics (astro-ph.EP) Chemical Physics (physics.chem-ph) Partition function (quantum field theory) Astronomy Astronomy and Astrophysics Function (mathematics) Astrophysics - Astrophysics of Galaxies Exoplanet Universe Interstellar medium Supernova Astrophysics - Solar and Stellar Astrophysics 13. Climate action Space and Planetary Science Astrophysics of Galaxies (astro-ph.GA) Astrophysics::Earth and Planetary Astrophysics Astrophysics - Earth and Planetary Astrophysics |
| DOI: | 10.48550/arxiv.1704.04096 |
| Popis: | H$_3^+$ is a ubiquitous and important astronomical species whose spectrum has been observed in the interstellar medium, planets and tentatively in the remnants of supernova SN1897a. Its role as a cooler is important for gas giant planets and exoplanets, and possibly the early Universe. All this makes the spectral properties, cooling function and partition function of H$_3^+$ key parameters for astronomical models and analysis. A new high-accuracy, very extensive line list for H$_3^+$ called MiZATeP was computed as part of the ExoMol project alongside a temperature-dependent cooling function and partition function as well as lifetimes for %individual excited states. These data are made available in electronic form as supplementary data to this article and at http://www.exomol.com Comment: 10 pages, 5 figures, 7 tables |
| Databáze: | OpenAIRE |
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