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Spectra of Hot Molecules of Astrophysical Importance: an Update on the ExoMol Project

Published online by Cambridge University Press:  21 February 2014

J. Tennyson  and
S. N. Yurchenko
J. Tennyson
Affiliation:
Department of Physics and Astronomy, University College London, London WC1E 6BT, UK
S. N. Yurchenko
Affiliation:
Department of Physics and Astronomy, University College London, London WC1E 6BT, UK
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Abstract

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The ExoMol project aims at providing comprehensive line lists of molecular transitions which are likely to be important in the atmospheres of extra-solar planets and cool stars, including brown dwarfs. The physics of the molecules involved varies and can be categories according to the number atoms in the species. Thus the molecules can be grouped as diatomics, both closed and open and shell, triatomics, tetratomics, methane and larger species. Progress in providing complete sets of line list for the molecules in each of these categorizes is considered. The latest line lists and related data for each of the species can be found on the project website www.exomol.com.

Keywords

molecular dataopacityastronomical data bases: miscellaneousplanets and satellites: atmospheresstars: low-mass
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S297: The Diffuse Interstellar Bands , May 2013 , pp. 330 - 338
Copyright
Copyright © International Astronomical Union 2014 

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