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  The Deep O/H Ratio in Uranus and Neptune from CO Spectroscopy and Thermochemical Modeling

Cavalié, T., Venot, O., Selsis, F., Hersant, F., & Hartogh, P. (2014). The Deep O/H Ratio in Uranus and Neptune from CO Spectroscopy and Thermochemical Modeling. Talk presented at Workshop on the Study of the Ice Giant Planets. Laurel, Maryland, USA. 2014-07-28 - 2014-07-30.

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Cavalié, T.1, Author              
Venot, O., Author
Selsis, F., Author
Hersant, F., Author
Hartogh, P.1, 2, Author              
Affiliations:
1Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832288              
2MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291              

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 MPIS_GROUPS:
 MPIS_PROJECTS: HERSCHEL: HIFI
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 Dates: 2014
 Publication Status: Not specified
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 Identifiers: BibTex Citekey: Cavalie:2014-213P
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Title: Workshop on the Study of the Ice Giant Planets
Place of Event: Laurel, Maryland, USA
Start-/End Date: 2014-07-28 - 2014-07-30

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