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The ExoMol Atlas of Molecular Opacities
by
Yurchenko, Sergei N.
, Tennyson, Jonathan
in
Accuracy
/ Brown dwarf stars
/ brown stars
/ Cool stars
/ Energy
/ ExoMol
/ exoplanets
/ Extrasolar planets
/ High temperature
/ Lists
/ molecular spectra
/ opacity
/ Planetary atmospheres
/ Spectrum analysis
/ Stars & galaxies
/ University colleges
2018
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The ExoMol Atlas of Molecular Opacities
by
Yurchenko, Sergei N.
, Tennyson, Jonathan
in
Accuracy
/ Brown dwarf stars
/ brown stars
/ Cool stars
/ Energy
/ ExoMol
/ exoplanets
/ Extrasolar planets
/ High temperature
/ Lists
/ molecular spectra
/ opacity
/ Planetary atmospheres
/ Spectrum analysis
/ Stars & galaxies
/ University colleges
2018
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While trying to remove the title from your shelf something went wrong :( Kindly try again later!
Do you wish to request the book?
The ExoMol Atlas of Molecular Opacities
by
Yurchenko, Sergei N.
, Tennyson, Jonathan
in
Accuracy
/ Brown dwarf stars
/ brown stars
/ Cool stars
/ Energy
/ ExoMol
/ exoplanets
/ Extrasolar planets
/ High temperature
/ Lists
/ molecular spectra
/ opacity
/ Planetary atmospheres
/ Spectrum analysis
/ Stars & galaxies
/ University colleges
2018
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Journal Article
The ExoMol Atlas of Molecular Opacities
2018
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Overview
The ExoMol project is dedicated to providing molecular line lists for exoplanet and other hot atmospheres. The ExoMol procedure uses a mixture of ab initio calculations and available laboratory data. The actual line lists are generated using variational nuclear motion calculations. These line lists form the input for opacity models for cool stars and brown dwarfs as well as for radiative transport models involving exoplanets. This paper is a collection of molecular opacities for 52 molecules (130 isotopologues) at two reference temperatures, 300 K and 2000 K, using line lists from the ExoMol database. So far, ExoMol line lists have been generated for about 30 key molecular species. Other line lists are taken from external sources or from our work predating the ExoMol project. An overview of the line lists generated by ExoMol thus far is presented and used to evaluate further molecular data needs. Other line lists are also considered. The requirement for completeness within a line list is emphasized and needs for further line lists discussed.
Publisher
MDPI AG
Subject
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