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ExoMol molecular line lists – XX. A comprehensive line list for H3+

Mizus, II; Alijah, A; Zobov, NF; Lodi, L; Kyuberis, AA; Yurchenko, SN; Tennyson, J; (2017) ExoMol molecular line lists – XX. A comprehensive line list for H3+. Monthly Notices of the Royal Astronomical Society , 468 (2) pp. 1717-1725. 10.1093/mnras/stx502. Green open access

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Abstract

H3+ 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 H3+ key parameters for astronomical models and analysis. A new high-accuracy, very extensive line list for H3+ called MiZATeP was computed as part of the ExoMol project alongside a temperature-dependent cooling function and partition function as well as lifetimes for excited states. These data are made available in electronic form as supplementary data to this article and at www.exomol.com.

Type: Article
Title: ExoMol molecular line lists – XX. A comprehensive line list for H3+
Open access status: An open access version is available from UCL Discovery
DOI: 10.1093/mnras/stx502
Publisher version: http://dx.doi.org/10.1093/mnras/stx502
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: molecular data, opacity, astronomical data bases: miscellaneous, planets and satellites: atmospheres
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery-pp.ucl.ac.uk/id/eprint/1551490
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